The galaxy appears as a moderately luminous, elliptical-like system, with a smooth, diffuse morphology dominating its overall structure. The light is primarily concentrated towards the center, with a gradual fall-off in intensity toward the edges. There are no apparent spiral arms, bars, or prominent dust lanes visible. The color gradient suggests a primarily older stellar population, as indicated by the reddish hue, with a possible slight bluer component within the core, suggesting a very recent and small burst of star formation. The galaxy's shape is somewhat elongated, appearing more "in-between" round and cigar-shaped, hinting at a non-spherical structure but not obviously disturbed or interacting. There is no visual evidence of major or minor mergers.
