The galaxy presents a smooth, elliptical morphology. It appears elongated, with a cigar-shaped profile. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars. The color appears more yellow/red-shifted, which potentially implies an older stellar population. No distinct spiral arms or prominent dust lanes are visible. The outskirts of the galaxy appear diffuse, gradually fading into the background. There is no obvious evidence of significant tidal disturbances or ongoing major merging activity, although a subtle asymmetry cannot be ruled out entirely. The overall appearance indicates a relatively evolved system with a low star formation rate.
