This galaxy presents a morphology that appears largely smooth, with a slight elongation. It is primarily elliptical in shape. There's a bright, concentrated central region, likely indicating a galactic bulge. A faint, diffuse halo surrounds the core, extending further along the galaxy's major axis. The color distribution suggests a mix of stellar populations. The central bulge exhibits a yellowish-white hue, potentially indicating older, cooler stars. The surrounding disk or halo region appears bluer, hinting at the presence of younger, hotter stars, and possibly some ongoing star formation, albeit at a low rate. Slight disturbances appear in the structure which may be a minor merger or tidal disruption. The overall structure suggests a system undergoing a relatively relaxed evolution.
