This galaxy exhibits a distinctly elongated, cigar-shaped morphology. The central region displays a high degree of smoothness and concentration of light, suggesting a significant bulge component. The galaxy's color appears generally redder, indicating a population dominated by older stars. There is limited evidence of spiral arm structure or significant dust lanes; however, a slightly bluer hue is visible toward the outer edges, potentially indicating some recent star formation, albeit at a low level. Overall, the galaxy appears to be relatively isolated, with no immediate signs of major mergers or tidal disturbances in the immediate vicinity. The lack of prominent features indicates the galaxy may be relatively evolved.
