The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth light distribution with no apparent spiral arm structures or dust lanes. The galaxy's light profile gradually decreases in intensity from the core outwards. There are hints of bluer colors in the central region, indicating the presence of possibly younger stellar populations. The outer regions seem to be redder, which might signify older stellar populations. There might be a very slight asymmetry, suggesting the presence of a possible minor disturbance, although the galaxy's overall appearance is largely undisturbed. It seems like a relatively massive galaxy with low star formation rate.
