The galaxy presents as a luminous, moderately elliptical structure with a smooth, concentrated central bulge. The dominant color is a yellow-red hue, suggestive of an older stellar population. Faint, diffuse features are visible extending from the main body of the galaxy, potentially indicating tidal disturbances or ongoing interactions. There appears to be evidence of a possible merger or interaction, suggested by the disturbed morphology and asymmetric light distribution. The lack of distinct spiral arms implies the galaxy is likely an elliptical or lenticular type, exhibiting a relatively quiescent star formation rate. Overall, the galaxy exhibits characteristics indicative of a relatively evolved system, perhaps undergoing a merging event.
