The galaxy presents as a relatively smooth, elongated structure, with a notable central bulge that appears yellowish, suggesting an older stellar population. Extending outwards from the central bulge, there are faint hints of a disk structure, but the disk is not well-defined and lacks prominent spiral arms. The color gradient transitions from a yellowish hue in the core to a slightly bluer tint in the outer regions, which may indicate some ongoing, albeit subdued, star formation. The galaxy exhibits a moderate degree of elongation, giving it a somewhat cigar-shaped appearance. No significant signs of recent or ongoing mergers or tidal disturbances are evident. Overall, it seems to be an early-type spiral or lenticular galaxy with a quiescent star formation rate.
