The galaxy presents a roughly elliptical shape with a bright, concentrated central bulge. The disk component exhibits a mottled texture. A slight asymmetry is observed in the distribution of light around the bulge, potentially indicative of tidal interactions or internal structures. The galaxy's color profile appears relatively uniform, suggesting a similar stellar population throughout, although the slight asymmetry may also influence this. There appears to be some disturbance and evidence of a potential minor merger event. Overall, the galaxy appears to be relatively smooth with a lack of distinctive features in the disk.
