The galaxy presents as a relatively smooth, elliptical or lenticular structure, displaying a centrally concentrated light profile. It shows a gradual decline in surface brightness from the core outwards, with no prominent spiral arms or distinct features. The color appears to be yellowish-white, suggesting a population of older stars, though there is a faint hint of bluer regions. There is no evidence of a recent major merger. The galaxy appears to be relatively isolated. The overall shape is more elliptical than disk-like, but is not perfectly round, and is not highly elongated.
