The galaxy presents as a largely smooth object with a slightly elliptical morphology. It exhibits a concentrated central bulge, visually dominant and appearing yellowish-orange, indicative of an older stellar population. The outer regions appear fainter and more diffuse, with a subtle color gradient suggesting a possible decline in star formation toward the outer edges. There is a slight hint of a disk structure, but it is poorly defined. Overall, the galaxy's morphology suggests a relatively evolved system. There appears to be little evidence of ongoing major mergers or significant tidal disturbances.
