The galaxy presents as a relatively smooth, elliptical object, appearing mostly featureless at this resolution. The light distribution is centrally concentrated, with a gradual decline in brightness outward from the core. The color appears to be primarily yellowish-white, possibly indicative of an older stellar population dominating its composition. The galaxy is slightly elongated, displaying a moderate degree of ellipticity. There are no discernible spiral arm structures or prominent dust lanes visible, suggesting it is likely an early-type galaxy. There is no evidence of any major ongoing merger activity or strong tidal disturbances affecting its overall morphology, although the possibility of minor interactions cannot be ruled out.
