The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a concentrated, bright core, appearing yellowish-orange in color, suggestive of an older stellar population. Moving outward from the core, the galaxy transitions to a slightly bluer hue, possibly indicating the presence of a younger stellar population in the outer regions, or perhaps low level star formation activity. There is no clear spiral structure or prominent dust lanes visible. Overall, the light distribution appears largely uniform. The galaxy exhibits a general round shape. There is no obvious visual evidence of major mergers or significant tidal disturbances in the immediate vicinity.
