This galaxy appears as a largely smooth, elliptical-like object with a concentrated central bulge. It is relatively round in appearance. There are subtle color gradients visible, with a slightly more yellowish hue towards the center, suggesting an older stellar population is dominating the core. The outer regions exhibit a bluer tinge, hinting at the presence of younger stars or ongoing star formation, albeit at a low rate. There are no prominent spiral arm structures or significant dust lanes visible, supporting a classification as an early-type galaxy. No signs of major mergers are apparent, although there may be a faint, subtle distortion in its outer halo, indicating potential past gravitational interactions. Overall, it presents as a moderately massive galaxy with a red shift of 0.266418, exhibiting signs of past star formation and some old stars.
