This galaxy presents as a relatively smooth object, appearing elliptical or lenticular in nature. It is primarily characterized by a central bulge of significant luminosity, which fades into a fainter, more diffuse halo surrounding it. There are no discernible spiral arm structures or prominent dust lanes visible in the image. The color profile suggests a population of older stars. Overall, the galaxy exhibits a moderate level of star formation. Based on the images, there does not seem to be any recent major mergers.
