The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core. There is a slight elongation, deviating from a perfect circular shape, but it does not exhibit a strongly cigar-shaped appearance. The overall color suggests a population of older stars, with a subtle gradient towards slightly bluer hues in the outer regions, hinting at possible recent star formation activity. No major disturbances or signs of ongoing mergers are readily apparent, though minor tidal features or faint interactions cannot be ruled out based on this image alone. 
