The galaxy presents as an edge-on spiral or lenticular type. A prominent, extended disk structure is observed, appearing relatively thin and elongated. The central bulge is bright and concentrated, exhibiting a somewhat smooth appearance. There is a color gradient across the galaxy, with the central regions appearing bluer and the outer regions becoming redder. This suggests a younger stellar population in the center compared to older stars in the outer disk. There is subtle indication of minor disturbance, such as slight asymmetry. Overall, there are no significant indications of a major ongoing merger.
