The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The color profile appears to be dominated by older stellar populations, inferred from the reddish-yellow hue. There is no visible spiral structure or dust lanes evident. The overall shape appears somewhat elongated, leaning towards a cigar shape, with no indication of tidal disturbances or ongoing merger activity. The galaxy's surface brightness decreases gradually from the center outwards, indicative of a relatively relaxed system with minimal recent star formation.
