The galaxy presents as a moderately luminous system with a smooth, elliptical morphology. It exhibits a concentrated, bright central bulge which appears yellow-white in color, suggesting a population of older stars. The galaxy's light gradually fades with increasing radius from the center, with the outer regions displaying a bluer hue. This may indicate the presence of younger stars in the galactic outskirts, although star formation appears quiescent overall. There is no evidence of significant tidal disturbances or ongoing mergers. The galaxy's overall structure appears relaxed and well-defined, with no prominent spiral arms or bar features visible.
