The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. Its overall shape is moderately elliptical, exhibiting a deviation from a perfect circle. There is a slight elongation without forming a clear, defined disk or bar structure.

The galaxy's color profile is primarily a pale blue-white, indicating a likely presence of younger, hotter stars. There is a suggestion of some substructure or irregularities within the primary body, as well as hints of minor disturbances in its morphology. No clear signs of spiral arms or pronounced dust lanes are observed. The galaxy does not appear to be undergoing a major merger.
