The galaxy presents as a largely featureless, smooth object with an elliptical morphology. There appears to be a concentrated central bulge with a yellow-orange hue, suggesting an older stellar population. This core region exhibits high luminosity. Moving outward from the center, the light gradually diminishes, displaying a more diffuse halo. There is a slight blue tinge to the outer regions, potentially indicating the presence of some younger, bluer stars. No distinct spiral arms or bar structures are discernible. There are no obvious signs of tidal disturbances or mergers. Overall, the galaxy appears to be relatively isolated and undisturbed.
