The galaxy presents as a relatively smooth, somewhat elliptical object. The central region exhibits a bright, concentrated core with a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy transitions to a less luminous, more diffuse region. Subtle color variations are present in the outer disk, with tinges of red and blue, indicating the presence of some younger stars and potential star formation. The overall structure appears largely undisturbed, with no obvious signs of a recent major merger or tidal disruption.
