The galaxy presents as a somewhat elongated, elliptical structure. Its light profile is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The core appears to be bright and yellowish, suggesting an older stellar population or significant dust obscuration. The outer regions show hints of a disk-like component with faint, diffuse arms or tidal features. There's a possible minor disturbance, indicating a past or ongoing interaction. The galaxy's color index shows a redder hue, particularly in the central bulge, possibly due to older stars or internal dust. Overall, it seems to be a large, relatively massive galaxy with a moderately low star formation rate.
