The galaxy presents as a smooth, elongated object. Its morphology appears to be disk-like but is seen at a highly inclined angle. There is a bright central bulge, concentrated towards the center, surrounded by a fainter, more diffuse halo. The light profile suggests an aging stellar population, with a generally reddish hue and a lack of prominent blue star-forming regions. There are no signs of a major merger event. The galaxy is slightly elongated in shape. There are no distinct spiral arms.
