The galaxy presents as an elliptical morphology, exhibiting a relatively smooth light distribution. The central region appears bright and concentrated, suggestive of a dense stellar population, and fades gradually into the outer regions, with no clearly distinguished spiral arm structures apparent. The ellipticity of the galaxy is moderate, elongated along its major axis. The galaxy exhibits a color gradient, with the central bulge appearing more yellow, while the outer regions appear slightly bluer. This color difference could indicate variations in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars being more prominent in the outskirts. There appears to be no evidence of significant dust lanes or tidal disturbances, suggesting a relatively relaxed, undisturbed system. The overall appearance indicates a galaxy that is likely undergoing passive evolution with a relatively low rate of star formation.
