The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, exhibiting a high degree of roundness. There is a central, bright core that gradually diffuses outward, with no distinct spiral arm structures or bar features apparent in the image. The color profile indicates a dominant population of older stars, as evidenced by the reddish-yellow hue, with a subtle hint of blue indicating a minor component of younger, hotter stars contributing to recent star formation. There is a minor disturbance possibly occurring, which could be a smaller galaxy merging into it. The absence of significant dust lanes and the smooth appearance suggests that this galaxy is in a relatively advanced stage of its evolution.
