The galaxy appears to be a relatively compact, lenticular or early-type spiral galaxy, seen at a high inclination. The light distribution is centrally concentrated and appears smooth, with little evidence of strong star formation. There is a suggestion of a faint, disk-like structure but no clear spiral arms visible. The major axis appears elongated, potentially classifying it as slightly cigar-shaped. There is some faint asymmetry in the outer regions, which may indicate minor gravitational interaction or a past merger event. The central bulge appears prominent. Overall, the galaxy exhibits characteristics indicative of an evolved system with a low star formation rate and a high degree of internal ordering.
