The galaxy presents a generally elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, suggesting a dominant bulge component. There is little evidence of distinct spiral arms or a prominent disk structure. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the central core, potentially indicating ongoing, albeit low levels of star formation at the edges. There might be some minor asymmetry or faint tidal features, hinting at past or ongoing interactions. These are not distinct. The overall appearance suggests a galaxy in transition, perhaps evolving from a more actively star-forming spiral to a more quiescent elliptical galaxy.