This galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a largely elliptical morphology. There is a distinct absence of well-defined spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region, potentially indicative of evolved stars. There appears to be a slight extension or tidal feature visible on one side of the galaxy, which may be the result of a minor gravitational interaction. Star formation activity is likely low. The overall appearance suggests a galaxy in the process of, or already having undergone, morphological transformation towards a more quiescent state. The galaxy appears isolated without any signs of major merging events, disturbances or interactions.
