The galaxy presents as a slightly elongated, lenticular-like system. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish-white hue, indicative of an older stellar population. The surrounding disk shows a bluer tint, suggesting more recent or ongoing star formation. The galaxy's disk appears relatively smooth, with some subtle indications of spiral arm structures. There may be faint disruptions in the outer regions of the galaxy, but it's difficult to confirm any merger events. Overall, the galaxy exhibits a moderate mass and star formation rate. It is primarily intermediate in shape, being neither perfectly round nor cigar shaped.