The galaxy presents as an elliptical-like morphology, characterized by a smooth, centrally concentrated luminosity profile. A distinct nucleus is observed, surrounded by a diffuse halo of lower surface brightness. The object exhibits a relatively compact apparent size and rounded shape, with the isophotes appearing largely regular. No prominent spiral arms, dust lanes, or other features indicative of active star formation are readily discernible in this imaging. The galaxy exhibits a reddish hue, possibly indicative of an older stellar population. There appears to be only minor disturbances visible, suggesting it is not undergoing a major merger with another galaxy.
