The galaxy appears as a concentrated, elliptical-like structure. There is a prominent, luminous core, surrounded by a more diffuse halo of light. The color profile suggests an older stellar population, with a dominant yellowish hue in the central region that fades outward into a slightly redder halo. No distinct spiral arms or significant dust lanes are visible. The galaxy has a smooth, featureless appearance, indicative of a relatively undisturbed system. There is no apparent evidence of any ongoing major mergers or tidal disturbances. Overall, the morphology suggests a well-formed, relatively quiescent galaxy.
