The galaxy presents as an elliptical shape with a high degree of central concentration. A bright, yellowish core region dominates the galaxy's luminosity profile, indicating an older stellar population likely residing within the bulge. Fainter, bluer light extends away from the core, suggesting the possibility of ongoing or recent star formation in the outer regions, although the rate appears to be very low overall. The galaxy exhibits a smooth texture, indicative of an evolved system with minimal dust lanes or spiral arm structures, though there appears to be a slight asymmetry on one side of the galaxy. The galaxy does not appear to be undergoing any major mergers or interactions, though there is a faint hint of tidal debris or a minor disturbance present. It has a moderate size, consistent with it being a smaller elliptical galaxy.
