The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears predominantly smooth, lacking any obvious spiral arm structures or significant irregularities. The light distribution suggests a high degree of rotational symmetry, with a near-circular isophotal shape. There's a subtle color gradient, with the central region exhibiting a slightly redder hue that transitions into bluer tones in the outer regions. No indications of ongoing major mergers or strong tidal interactions are apparent from its morphology. Subtle disturbances or minor interactions cannot be ruled out, but the dominant impression is that of a relatively undisturbed system.
