The galaxy presents an elliptical morphology, appearing mostly smooth with minimal discernible features, such as spiral arms or dust lanes. The light distribution appears centrally concentrated. There is an indication of a slight elongation, deviating from a perfect circular shape. The galaxy displays a color gradient, transitioning from a slightly bluer hue in its outer regions to a more pronounced yellowish-red core. This color difference suggests a variation in stellar population, potentially with younger, hotter stars in the periphery and older, cooler stars concentrated in the central bulge. There appears to be no major mergers or significant tidal disturbances. The lack of strong blue color and the overall smooth appearance suggest a relatively passive or quiescent state of star formation.
