The galaxy presents as a well-defined, elongated structure, suggesting an elliptical morphology or a spiral galaxy viewed at a significant inclination. There is a noticeable concentration of light toward the center, with a smooth, diffuse profile extending outward. The core exhibits a yellowish-white hue, potentially indicative of an older stellar population dominating the central regions. Fainter, bluer outskirts suggest the presence of younger stars and/or ongoing star formation, albeit at a relatively low rate. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. The general form of the galaxy is somewhat cigar shaped.
