The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core region exhibits a yellow hue, suggesting a population of older stars. Fainter, extended regions surrounding the core are visible, with a slight hint of bluer light. This may be indicative of some ongoing, albeit relatively low, star formation activity in its outer reaches. No prominent spiral arms or significant dust lanes are discernible. The overall structure appears relatively undisturbed, without any obvious signs of recent major mergers or tidal interactions.
