The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology, showing a high degree of radial symmetry. A bright central bulge dominates the structure, transitioning into a more diffuse halo. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The overall color profile suggests a population of older stars, with a slight blueish tinge in the outer regions. There is no evidence of active merging or significant tidal disturbances affecting the galaxy's morphology. Overall, it is a well-defined object with a smooth luminosity profile.
