The galaxy presents as a slightly elongated, elliptical form. Its color profile indicates a dominance of older stellar populations, emitting primarily in the redder wavelengths. The morphological assessment suggests it is a smooth galaxy with a cigar shape, and it is not undergoing a major merger. There appears to be a minor disturbance, possibly a small tidal tail or faint nearby object, that is slightly bluish in hue. The overall structure is smooth and relatively featureless, typical of an early-type galaxy.
