The galaxy presents as a generally smooth, rounded structure. Its core exhibits a bright, concentrated luminosity, indicative of a high density of stars, and potentially an active galactic nucleus. A slight ellipticity is observed, suggesting the galaxy may be an elliptical galaxy. There appears to be a slight asymmetry in the light distribution, potentially signaling a minor gravitational disturbance. The overall color is indicative of an older stellar population, with some regions showing bluer hues. It seems unlikely that there is currently a major merger. 
