The galaxy appears as a slightly elongated, lenticular or early-type spiral system. It exhibits a generally smooth morphology with no readily discernible spiral arm structure. The central bulge is a prominent feature, displaying a yellowish hue, possibly indicating an older stellar population and a concentration of stars towards the galactic center. The disk component appears bluer, suggesting the presence of younger stars and ongoing star formation, though at a relatively modest rate. There is a slight hint of a disk-like structure extending outwards from the bulge, with a fuzzy, indistinct boundary, lacking sharp definition, which could indicate it is an older, more evolved galaxy. There's no visual evidence of any major ongoing mergers or strong tidal disturbances. A slight asymmetry to the galaxy's outer regions suggests minor interactions may have occurred in the past, or a possible minor merger. Overall, this galaxy presents the characteristics of a relatively massive and mature system undergoing moderate star formation.
