The galaxy presents as an elliptical morphology, appearing relatively smooth in texture. It exhibits a central bulge that is bright and concentrated, with luminosity decreasing gradually towards the outer edges. The overall color suggests an older stellar population, potentially with ongoing but low levels of star formation. The galaxy is elongated, approaching a cigar shape. There is no evident disk structure or spiral arm features visible. It appears to be isolated, with no signs of major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out.