The galaxy presents as an elliptical structure with a dominant, smooth morphology. The central region exhibits a high concentration of luminosity, appearing bright and yellowish-orange, suggesting a population of older stars. Moving outwards from the core, the luminosity decreases gradually, maintaining a relatively uniform color gradient without noticeable distinct features such as spiral arms or prominent dust lanes. The overall shape is close to round, with minimal elongation. There is no significant evidence of recent or ongoing major mergers or tidal disturbances in the immediate vicinity. The color profile indicates a likely absence of significant recent star formation.
