The galaxy presents an intermediate morphology, with a notable fraction exhibiting smooth features, although a disk-like structure or other distinct features are discernible. There appears to be some minor disturbances in the structure, yet the overall form does not indicate a major merger event. The galaxy has a moderate size and appears somewhat flattened. A slight asymmetry is present, suggesting some interaction or internal dynamics. The overall color is yellowish-white, which indicates it is likely a population of older stars. There are also hints of bluer regions that might be evidence of ongoing star formation activity, although it is not pervasive. Given the estimated absolute magnitudes, the galaxy is intrinsically luminous.
