The galaxy presents a moderately elongated, cigar-shaped morphology. A dominant smooth component is observed, with what appears to be a relatively small disk like or featured component. The central region displays a concentrated, bright luminosity, potentially indicative of an active galactic nucleus or a dense stellar population. The galaxy exhibits a color gradient, transitioning from a bluer hue at the edges to a redder, yellow-ish tint towards the central bulge. The arms of the galaxy appear relatively smooth, not flocculent, with faint dust lanes or spiral arm structures visible. There's no obvious evidence of a recent major merger. Overall, the galaxy looks like a relatively massive system with a mature stellar population.
