The galaxy presents as a relatively smooth, elliptical morphology with a bright, concentrated central bulge. The light distribution appears largely uniform, with a gradual decrease in intensity from the core outwards, suggesting an older stellar population. A faint, somewhat flattened disk is observed surrounding the bulge. It shows a slight inclination, possibly a near face-on view, and is characterized by a yellow-red color. There is no obvious spiral structure, suggesting the galaxy is not actively forming stars at a high rate. No signs of tidal disturbances or ongoing mergers are apparent, although some asymmetry in the outer halo cannot be ruled out. Overall, it is a compact, early-type galaxy with evidence of an aging stellar population.
