The galaxy presents a generally smooth morphology, with a centrally concentrated light distribution. The overall shape is somewhat elliptical, appearing more elongated than perfectly circular, though it lacks a pronounced disk structure. There is a notable color gradient, with a yellowish hue dominating the central region, suggesting an older stellar population. Fainter, reddish extensions are visible on one side, possibly indicative of minor tidal disturbances or ongoing star formation in the outer regions. The galaxy does not display any strong evidence of active merging or major disruptions.
