The galaxy presents a generally smooth, elliptical morphology. Its core region exhibits a bright, concentrated luminosity, suggesting a high stellar density, likely dominated by older stellar populations. The galaxy's color gradients suggest some variation in stellar populations or dust content. The galaxy appears fairly isolated, with no obvious signs of major mergers or significant tidal interactions. There is a slightly dimmer region within the halo of the galaxy. It presents a slightly elongated structure. There are no readily apparent spiral arms or disk-like features.
