The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is largely elliptical in appearance, with no immediately discernible spiral arm structure or pronounced disk features. The light distribution exhibits a radial gradient, with the brightest region concentrated in a small, unresolved core. This central region is surrounded by a more diffuse halo that fades gradually into the background sky. 

There is a slight elongation to the overall shape, but the galaxy is generally quite rounded. The color profile suggests a population of older stars, with a yellow-red hue dominating the central regions. A faint blue tinge is perceptible in the outer regions of the halo. There's no obvious evidence of ongoing major mergers or tidal disturbances in this image, although a subtle asymmetry may indicate a minor interaction.
