The galaxy presents as a concentrated, elliptical-like form, exhibiting a notable central bulge. The light distribution appears relatively smooth and consistent, with a high degree of symmetry. The galaxy core shows high luminosity. Color gradients suggest the presence of older stellar populations dominating the central regions. The galaxy appears to be in a possible merger state, indicated by a companion galaxy. There are faint signs of minor tidal disturbances. Overall, the galaxy has a redder hue, possibly indicative of an older stellar population. The galaxy is relatively compact, appearing to be a small galaxy.