The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears centrally bright with a gradual falloff outwards. The galaxy exhibits a mostly elliptical morphology, appearing largely rounded. There is little evidence of spiral arm structure or significant dust lanes. The color is broadly consistent with an older stellar population. There is little to no sign of strong recent star formation. I note subtle irregularities in the outer light distribution, hinting at a possible weak tidal interaction or disturbance, although this requires further investigation.
