The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated light profile. There is a distinct lack of spiral arm structures or prominent dust lanes. The overall shape approximates a flattened spheroid, tending toward round. The central bulge is bright and concentrated, suggesting a dense stellar population. Color gradients indicate a population of older stars. The galaxy does not appear to be undergoing a major merger or exhibiting strong tidal disturbances. Faint extensions or diffuse halos may exist, but are not distinctly resolved in this image. There may be slight asymmetries visible, which could be due to a minor disturbance or subtle tidal interactions. Star formation activity appears low, consistent with a redder color index. 
