The galaxy appears as a centrally concentrated object with a somewhat smooth morphology. It exhibits a roughly elliptical shape, though not perfectly circular, tending towards a more flattened, "in-between" profile. The central region displays a yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse greenish light extends outwards from the core, possibly indicating the presence of some ongoing, albeit low-level, star formation within the galaxy. There is no obvious sign of spiral arm structure or a well-defined disk. The outer regions fade gradually into the background, showing no significant signs of tidal disturbances or major mergers. Overall, the galaxy's light distribution is relatively even and featureless.
