The galaxy presents as a luminous, elliptical object. Its morphology appears predominantly smooth with a high degree of central concentration. There is little discernible structure such as spiral arms or prominent dust lanes. The object exhibits a moderate degree of ellipticity, appearing slightly elongated rather than perfectly spherical. The color profile suggests a population of older stars, with a yellowish-red hue dominating the visual spectrum. The overall impression is that of a relatively quiescent system, potentially with low ongoing star formation. There is no indication of any major interaction with another galaxy or any ongoing merging event. The galaxy appears to be an isolated system.
