The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a population of older stars, indicated by the reddish-yellow hue, particularly prominent in the central regions. There is a possible tidal feature or a minor companion galaxy, but the image is too grainy to tell for sure. If it is a companion galaxy, it appears to be a smaller, fainter object also reddish-yellow. The main galaxy exhibits a radial light distribution that decreases smoothly outward from the core. No discernible dust lanes or spiral arm structures are visible. The overall appearance indicates a system that has likely undergone significant dynamical relaxation and/or morphological transformation, potentially resulting in the suppression of star formation within the main galactic body.
