The galaxy presents as a centrally concentrated object with a generally elliptical morphology. The core region exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. The light fades gradually outwards from the core, transitioning to a bluer hue in the outer regions of the galaxy. This may indicate some recent star formation on the galactic outskirts. No significant spiral arm structure or dust lane features are obviously apparent within this galaxy, nor do any tidal disturbances or merging characteristics stand out. The smooth appearance implies the galaxy is relatively undisturbed, with the light being almost uniform in its dispersion and structure. It appears to have a moderate size.
