The galaxy appears to be a relatively compact system with a centrally concentrated light profile. The overall morphology suggests a spheroid shape, possibly elliptical. There is no strong evidence of spiral arms or a distinct disk component from this viewing angle. Color gradients are subtle but indicate a possible redder core and bluer outer regions. The light is primarily concentrated in a central bulge, with a slight extension in one direction that could indicate a minor tidal disturbance or ongoing merger. There are no prominent dust lanes visible within the galaxy, and the overall structure appears relatively smooth and undisturbed, although with a high likelihood of being impacted by some type of merger.
