The galaxy presents as a relatively bright, lenticular-like structure with a concentrated central bulge. A diffuse disk is apparent, exhibiting a subtle blue hue, possibly indicative of ongoing star formation. While the object displays a generally smooth appearance, a slight distortion or faint tidal feature might be present on the edges, suggesting past or ongoing minor gravitational interaction. The galaxy is moderately round in shape, although it has a few irregularities. The integrated light suggests a mature stellar population in addition to ongoing star formation.
