This galaxy presents as a somewhat elliptical, moderately luminous object. The central region exhibits a concentrated, bright core, suggesting a significant density of stars and potentially a supermassive black hole actively accreting matter. Surrounding the core, there is a more diffuse, extended halo. The color gradient transitions from a yellowish-white in the core to a bluer hue in the outer regions of the halo, indicating the presence of younger, hotter stars in the outer regions, though the bluer colors may be weak. There may be little to no indication of spiral arm structure, and it appears to be a relatively undisturbed system, lacking any obvious signs of major mergers or tidal distortions. It is primarily smooth in texture, suggesting a well-mixed stellar population.
