The galaxy presents as a centrally concentrated, elliptical form. It appears relatively smooth in texture, with a gradual decrease in luminosity from the core outwards. The core region exhibits a pinkish hue which possibly suggests a population of older stars. There is some bluer light surrounding this central region, implying the presence of a younger stellar population, but it is less defined. A subtle, but extended, diffuse halo is visible, suggesting potential interactions or past merger events, but it is difficult to discern. The primary orientation of the galaxy is tilted slightly, deviating from a perfect circular profile. Overall, there is no strong evidence of intense star formation activity.
