This galaxy presents a morphology that suggests a relatively evolved system. The light distribution is centrally concentrated, indicating a significant bulge component. The elliptical isophotes are nearly round and suggest it is a relatively smooth elliptical galaxy. A hint of disk-like structure is present, but it is not very prominent.

The color gradient observed shows a gradient, with the central region appearing bluer than the outskirts. The observed colors also suggest the presence of an older stellar population, with moderate ongoing star formation. The galaxy's size is moderate compared to other galaxies observed, neither exceptionally large nor particularly compact. There may be some tidal features.
