The galaxy presents a largely smooth, elliptical morphology. Its light distribution appears relatively uniform, with a concentration toward the galactic center, but without prominent spiral arms or a distinct disk structure. The color profile suggests a dominant population of older stars, giving the galaxy a reddish-yellow hue. There are subtle hints of fainter, bluer light in the outer regions of the galaxy, possibly indicating regions of residual star formation. Overall, the galaxy appears to be a relatively massive system that has largely ceased active star formation. There is no evidence of ongoing major mergers or significant tidal disturbances.
