The galaxy presents as a smooth, elongated structure indicative of an elliptical morphology. The core region is relatively bright, appearing concentrated and lacking in discernible substructure. Moving outward from the core, the luminosity gradually diminishes, forming a diffuse halo that extends along the major axis. The overall color profile appears relatively uniform, dominated by yellowish hues, suggesting a population of older stars. There is no evidence of spiral arms or significant dust lanes. Minimal or no ongoing star formation is apparent within the galaxy. The galaxy appears undisturbed, showing no signs of a major merger or significant tidal interactions.
