The galaxy presents as a relatively smooth, elongated structure, likely a lenticular or elliptical type. It exhibits a strong central bulge which appears to have a yellowish hue, suggesting an older stellar population. The outer regions appear to be significantly bluer than the central region, suggestive of more recent star formation within an extended disc. There are indications of a possible faint dust lane in the central region of the galaxy, contributing to the central color variations. The galaxy exhibits a cigar-like morphology, with the major axis being significantly longer than the minor axis. Overall, the galaxy appears relatively undisturbed, showing no signs of recent major mergers or tidal interactions.