The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape though not perfectly so. It exhibits a bright, concentrated central bulge with a gradual decrease in luminosity outwards. There is a hint of asymmetry, possibly indicating a minor disturbance or interaction. A faint tidal tail or extended structure is visible extending away from the galaxy, suggesting a past merger event or ongoing interaction with another galaxy. The color profile appears relatively uniform across the galaxy, with a yellow hue. This implies a population of older stars and a low star formation rate throughout the galaxy. There is an irregular component located above the center mass. This could be a cloud or irregular galaxy in the process of merging with the main galaxy.
