The galaxy presents an elliptical morphology, although with noticeable irregularities, indicating a potential ongoing or recent merger event. A dominant central bulge, characterized by a yellowish-orange hue, is visible. Faint blue wisps extending from the central region suggest areas of younger stellar populations. The overall light distribution is diffuse. The galaxy exhibits low star formation activity. Evident from its slightly perturbed shape, it could be undergoing interactions with a smaller companion galaxy. There is a minor disturbance in the galactic structure. The galaxy appears to be relatively massive, with the likelihood of containing a supermassive black hole at its core.
