The galaxy presents as a relatively compact, elliptical or lenticular system. Its overall structure exhibits a smooth, centrally concentrated light distribution, indicative of an evolved stellar population. There is a suggestion of a slightly elongated form. The color profile appears moderately red, pointing toward a population of older stars with limited on-going star formation. No prominent spiral arms or distinct morphological features are discernible. There is no obvious sign of any ongoing merger activity or any major disturbances within the galaxy's structure.
