The galaxy appears to be relatively compact with an estimated radius of approximately 5 arcseconds. Morphologically, the galaxy exhibits a primarily smooth structure with only minor irregularities. The overall color profile suggests a population of older stars, indicated by a more pronounced presence of red light relative to blue. There is a potential for minor tidal disturbances, with a slight asymmetry or faint plume-like feature extending from the main body of the galaxy. The galaxy is likely an elliptical galaxy, with the possibility of being in a minor merging state, as suggested by subtle structural distortions.
