The galaxy appears as a system with multiple components. A primary, central object is roughly elliptical in shape, displaying a smooth, diffuse light profile. Its core exhibits a concentration of older stellar populations, indicated by the orange-red hue. Extending outward from this core, faint traces of what might be a disk-like structure are visible, tinged with a hint of blue, suggesting the presence of some younger, hotter stars, even if the overall star formation rate is relatively low. A secondary object is apparent on the side, possibly a companion galaxy or a region of active star formation within the primary galaxy. This smaller object shows a distinct redder color, which may be indicative of an older stellar population or a higher dust content. There are no obvious signs of major tidal disturbances or ongoing major mergers; however, the subtle distortions present could indicate minor gravitational interactions or past merger events. The galaxy's morphology points towards a transition state, possibly evolving from a spiral towards an elliptical or lenticular form, given the partially smooth structure and suppressed but present star formation.
