This galaxy appears to be a single, fairly luminous object at a considerable distance. Morphologically, it presents as a relatively smooth system. While there is some indication of substructure, it lacks a prominent disk or spiral arms. The overall shape tends toward round, exhibiting low ellipticity. The central region displays a condensed, brighter core surrounded by a more diffuse halo. There is evidence of minor disturbances in the galaxy's morphology, but no indication of a major ongoing merger. The color suggests that it has a population of stars, likely intermediate to old in age, and exhibits signs of ongoing star formation.
