The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light profile. The core exhibits a yellowish-white hue, suggesting a population of older stars. The isophotes are generally round, with a slight tendency toward ellipticity. There is a faint blueish tinge on the outer edges of the galaxy's disk, suggesting the presence of some younger, hotter stars, though these are minimal compared to the overall stellar population. There are no apparent spiral arm structures or significant dust lanes visible. Overall, this galaxy presents as a relatively undisturbed, mature system.
