This galaxy exhibits a generally smooth morphology, although some features suggest possible tidal interactions or disturbances. It appears to be neither perfectly elliptical nor a clear spiral. The core region shows a concentration of light, appearing bright and yellowish, which could indicate an older stellar population with less active star formation in the central regions. There are faint, diffuse extensions of light surrounding the main body of the galaxy, suggesting a possible halo of stars or a disturbed outer structure. Overall, the morphology is suggestive of a system that may be in the process of merging or has undergone a merger in the recent past, evidenced by the irregular shape and luminosity distribution.
