The galaxy presents a smooth, elliptical morphology. The central region exhibits a concentrated luminosity, appearing almost spheroidal in shape. The light distribution gradually diminishes outwards, suggesting a centrally-dominated stellar population. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears largely undisturbed, showing no strong signs of ongoing merger activity. The color profile indicates a generally evolved stellar population, leaning towards older stars. A minor amount of blue is present in the surrounding area. The galaxy appears fairly isolated with no companion galaxies nearby.
