The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical in nature, displaying a rounded form with no discernible spiral arms or bar structures. The galaxy exhibits a color gradient, appearing yellower toward the center and becoming slightly bluer in the outer regions. This suggests the central region may contain an older stellar population, while the periphery might have more recent star formation.

There is no apparent ongoing major merger activity or significant tidal disturbance, although a minor asymmetry cannot be ruled out. The overall structure indicates a mature system, likely having undergone significant evolution. Further spectral analysis is required to definitively confirm the stellar populations and star formation rates.
