The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is no distinct spiral arm morphology visible. The core is bright and exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy display a gradual decrease in luminosity, transitioning from yellow to reddish tones, indicative of a mixture of older stars and dust absorption. The galaxy appears moderately rounded, lacking significant elongation or asymmetry. There is no obvious evidence of ongoing major mergers or tidal disturbances; however, the irregular color distribution and overall morphology hint at possible minor interactions or internal activity.
