This galaxy presents as a somewhat amorphous, though generally elliptical, structure. The light is concentrated towards the center, exhibiting a bright, diffuse core with a yellow-orange hue, suggesting an older stellar population. Fainter, bluer light extends outward from the core, possibly indicating areas of more recent, though moderate, star formation. There is a slight asymmetry to the galaxy’s outer edges, but no clear evidence of spiral arms or a prominent disk. The overall appearance suggests a galaxy that is neither purely elliptical nor clearly spiral, but perhaps an intermediate form, or a disk galaxy with a significant bulge component. There is a hint of potential tidal disturbance or interaction in the subtle asymmetry, though not strongly indicative of a major merger event.
