The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a significant inclination. A distinct central bulge exhibits a concentrated, yellowish-orange hue, suggestive of an older stellar population. The disk component appears relatively smooth, with a subtle bluish tint on its periphery, possibly indicating regions of more recent, albeit limited, star formation. There is no obvious evidence of strong spiral arm structures or active star-forming regions typically associated with later-type spiral galaxies. The galaxy's elongated shape and smooth light distribution imply a relatively evolved system, potentially transitioning toward a more elliptical morphology. The overall appearance suggests a massive system with a substantial stellar mass. No obvious signs of ongoing major mergers or strong tidal interactions are apparent.
