The galaxy presents as a somewhat elliptical, lenticular morphology. The central bulge is bright and concentrated, displaying a yellowish hue, suggestive of an older stellar population. There is a faint, diffuse disk extending outwards. The light distribution appears relatively smooth with no clear spiral arm structures. A subtle bluer tint is seen within the disk. The disk is elongated. The overall structure suggests that the galaxy is dominated by an old stellar population with very little ongoing star formation. There is a notable lack of dust lanes.
