The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution. It presents an ovoid shape, slightly elongated rather than perfectly spherical. The core region displays a bright, concentrated glow, suggesting a high density of stars. Moving outwards from the center, the luminosity gradually decreases, with no distinct spiral arms or prominent features visible. The galaxy appears relatively undisturbed, without significant signs of ongoing mergers or tidal interactions. The color gradient indicates a population of older stars dominating the stellar content. Overall, it seems to be a relatively massive galaxy.
