The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, characterized by a yellowish-white hue, suggesting an older stellar population. The overall color gradient transitions towards a bluer periphery, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation in the outer regions. The galaxy exhibits a moderate degree of roundness, deviating slightly from a perfectly circular shape. There are no obvious signs of major mergers or significant tidal disturbances, although some minor asymmetry in the outer regions cannot be entirely ruled out. The relatively compact size suggests that the galaxy has a moderately high mass. The blue tinge may also be influenced by a relatively low rate of ongoing star formation, although the dominant color suggests that it has mostly older stars. Overall, it appears to be an elliptical galaxy with a modest degree of star formation in its outer regions.
