The galaxy presents as a generally smooth, elliptical structure with a concentrated central bulge. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core outwards. The galaxy exhibits a yellow-white hue in its central region, suggesting a population of older stars. Fainter blue-ish tones are present in the outer regions, potentially indicating some ongoing, albeit low, star formation. No spiral arms, distinct dust lanes, or signs of recent major merger activity are readily apparent. There might be very slight asymmetry to its shape, but overall it appears well relaxed.
