This galaxy presents an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The light distribution suggests a relatively old stellar population, contributing to its yellowish-gold hue. There is a notable lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, showing no signs of ongoing major merger activity or significant tidal distortions. The overall smooth appearance suggests a system dominated by a spheroidal component with little ongoing star formation. The galaxy's elongated shape, but without a strong disk component, indicates it is likely an elliptical galaxy of intermediate ellipticity.
