The galaxy presents as a relatively smooth, elliptical structure. There is a concentration of light toward the center, suggesting a prominent galactic nucleus. The color profile appears relatively uniform across the galaxy, with a slight shift towards the redder end of the spectrum, particularly in the central regions. The galaxy has a generally round morphology, with no apparent significant distortions or tidal features indicative of major merger activity. Faint extended light is observed, potentially indicating a diffuse halo or stellar population surrounding the galaxy. There are some subtle irregularities, but overall, the structure is regular and appears to be relatively undisturbed. Based on its color, the galaxy appears to be relatively red, which is consistent with a more evolved stellar population and lower rates of active star formation.
