The galaxy presents as a centrally concentrated, elliptical-like structure. There appears to be a smooth, spheroidal component dominating the light profile. The central region exhibits a high surface brightness, with a gradual fading of light intensity towards the outer edges. The color profile suggests a population of older stars, as indicated by the yellowish-red hue concentrated towards the center, potentially due to the presence of red giant stars and a lower abundance of young, blue stars. The galaxy does not show prominent spiral arms or a distinct disk-like structure. There are no signs of significant ongoing mergers or major disturbances in its morphology; however, the shape is somewhat elongated, indicating it is likely not perfectly spherical. Overall, this galaxy appears to be a relatively evolved system.
