The galaxy presents an elliptical morphology, with a smooth and centrally concentrated light distribution. The core region exhibits a yellowish hue, suggestive of an older stellar population, likely dominated by red giant stars. The light intensity gradually decreases outwards, transitioning into a fainter, diffuse halo with a slightly bluer color. There appears to be only very minor disturbances to the general shape of the galaxy; no distinct spiral arm features are visible, nor is there any other evidence of ongoing or recent major merger activity. The galaxy's elongated shape indicates it is an oblate spheroid, seen from a somewhat inclined viewing angle.
