The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely featureless, with a gradual decrease in surface brightness towards its outer regions. The color profile suggests a dominant older stellar population, with a yellow to orange hue in the central regions transitioning to a slightly bluer tint further out. There appears to be very little evidence of active star formation, based on the color and lack of distinct spiral arms or prominent HII regions. It is generally a round object, with the possibility of very minor disturbances from surrounding objects.
