The galaxy exhibits a predominantly smooth morphology, with a centrally concentrated bulge that dominates the overall structure. The shape appears to be somewhere between round and elliptical. Faint, diffuse outer regions are present, extending slightly beyond the brighter central region. No distinct spiral arm features or other prominent disk structures are readily apparent, and there is no evidence of strong tidal distortions or ongoing major mergers. The color gradient suggests the presence of a relatively old stellar population, with redder hues concentrated towards the core, potentially indicative of a lack of significant recent star formation activity. Minor irregularities can be seen at the edge of the galaxy.
