The galaxy presents a generally smooth, elliptical morphology. It exhibits a somewhat elongated shape, appearing more cigar-shaped than perfectly round. The core of the galaxy is noticeably brighter and exhibits a yellowish hue, which suggests a population of older stars dominating its composition. There is little evidence of spiral arm structure or distinct disk features. The lack of blue light indicates minimal ongoing star formation, pointing toward a quiescent or passive evolutionary state. The overall color is redder, confirming the dominance of an older stellar population. No apparent signs of tidal disturbances, mergers, or significant morphological irregularities are observed. The galaxy appears relatively isolated and undisturbed.
