The galaxy presents as a somewhat elliptical structure with a dominant, smooth central bulge. The core region exhibits a concentrated yellowish-white color, suggesting a population of older stars. Surrounding the core is a fainter, less defined disk or halo, appearing mottled with subtle variations in color. Bluer hues, possibly indicative of more recent star formation, are observed in the outer regions, though they do not form distinct spiral arms or features. There is a slight irregularity to the overall shape, with a hint of disturbance or interaction. The galaxy appears relatively isolated, without evidence of major ongoing mergers or tidal disruptions, though minor disturbances are visible. The shape is somewhere between round and elongated.
