The galaxy presents as an elliptical-like system, with a moderately bright central bulge. The primary body of the galaxy exhibits a flattened morphology. There appears to be a slight color gradient, with the core region displaying a yellowish-white hue, suggesting an older stellar population. Fainter bluish-white regions extend from the central bulge along the major axis, indicating some presence of younger, hotter stars or ongoing star formation, however, the galaxy is for the most part composed of older stars. The edges of the galaxy fade into the background sky, indicating a smooth transition in stellar density. No distinct spiral arm structures or strong dust lanes are observed. There is some marginal evidence of tidal disturbances or interactions.
