The galaxy presents a generally smooth morphology, with a notable absence of spiral arm structure. The light distribution suggests it is elliptical in shape, elongated along its major axis. A bright, concentrated central bulge is evident, fading outward into a more diffuse halo. The color appears to be predominantly composed of older stars, with a slight shift toward bluer hues, possibly indicating a moderate level of ongoing star formation within the galaxy. There are no signs of significant tidal disturbances or ongoing mergers.
