The galaxy appears as a relatively smooth, elliptical-like structure. There is a slight elongation, with the ratio of the major to minor axis approaching approximately 2:1, but it is generally round in appearance. The color is mostly a homogenous yellowish-orange hue, which suggests an older stellar population with minimal ongoing star formation. The overall light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the outer edges. There are hints of some irregularities or minor disturbances in the light profile that are not easily discernable, perhaps an indication of past interactions. The galaxy's structure is not clearly defined as a disk or spiral system; however, a smooth disk cannot be ruled out with the available data. There is no evidence of a recent major merger event, though minor interactions seem likely. Overall, the galaxy appears to be a relatively evolved system nearing quiescence.
