The galaxy presents a mostly smooth morphology with a slightly elliptical shape. The light distribution appears to be concentrated towards the center, with a bright, yellowish core indicative of an older stellar population. The outer regions show a gradual decrease in luminosity, transitioning to a fainter, more diffuse halo with a slightly bluer hue. No distinct spiral arms or prominent dust lanes are visible, suggesting it is likely an early-type galaxy. There is no apparent sign of any major disturbance or merging event.
