The galaxy appears to be an elliptical or lenticular type, with a smooth, diffuse light distribution and lacking prominent spiral arms. The central bulge is noticeable but not overly dominant. Its overall shape is moderately elongated rather than perfectly spherical.

The color index suggests the presence of a stellar population that is more evolved, with a bias towards older, redder stars. Star formation activity is either low or absent. There appears to be a possible minor disturbance, but it is not significantly disrupted.

The galaxy exhibits a relatively compact size, suggesting a moderate luminosity. There is no obvious presence of an active galactic nucleus (AGN). There are no surrounding tidal tails or debris.
