The galaxy presents as a centrally concentrated, luminous object with a largely smooth morphology. It appears elliptical in shape, with a high degree of roundness. There are no prominent spiral arms or distinct bar structures visible. The galaxy exhibits a color gradient, with a yellowish core suggesting an older stellar population and a bluer, diffuse halo indicating the presence of younger stars or ongoing star formation within the outer regions. There are no obvious signs of tidal interactions or major disturbances, implying a relatively isolated and quiescent system. The galaxy appears to be in a non-merging state, without evidence of significant morphological disruptions, or intense starburst activity.
