The galaxy presents as a luminous, elliptical-shaped structure with a smooth, diffuse profile. Its core exhibits a concentrated, bright yellow hue, suggesting a dense population of older stars. The light gradually fades towards the outer regions of the galaxy, maintaining a consistent yellowish color, indicative of an evolved stellar population. The lack of distinct spiral arms or prominent dust lanes suggests a relatively quiescent galaxy, potentially with ongoing, albeit low, star formation activity. There is some evidence of a potential minor interaction or merger event. The morphology appears largely undisturbed, yet there is some degree of asymmetry observed, possibly indicative of gravitational interactions.
