The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a centrally concentrated luminosity profile. The central region is bright and yellowish-white in color, suggesting an older stellar population. There is a subtle decrease in brightness outwards from the center towards the edges. The galaxy is more or less round. There is no obvious evidence of distinct spiral arms or prominent dust lanes. The galaxy appears relatively undisturbed with no signs of a major ongoing merger, though there is potentially some minor asymmetry or distortion. Based on its red color, it is consistent with a relatively massive galaxy with a modest star formation rate.
