The galaxy presents as a luminous, centrally concentrated system. The overall morphology appears to be elliptical, although the outer regions exhibit a less defined structure. The core region is intensely bright, suggestive of a high stellar density or potentially an active galactic nucleus. Proceeding outward from the core, the light intensity gradually decreases. Faint extensions of diffuse light are visible, indicating the presence of a more extended halo. There is a slight asymmetry present in the outer regions which may suggest a past or ongoing interaction. The galaxy exhibits a reddish hue, which could indicate an older stellar population with lower rates of star formation. 
