The galaxy presents as a smooth, elliptical-like structure. The central region exhibits a concentrated, luminous core with a yellowish hue, suggesting a population of older stars. The overall shape is elongated, appearing somewhere between round and cigar-shaped. There is no readily apparent spiral arm structure or significant dust lane obscuration. The galaxy displays a largely undisturbed morphology, with no significant signs of ongoing or recent major merger events. Subtle color variations might indicate some low-level star formation activity.
