The galaxy appears as a single, relatively smooth and concentrated structure. It exhibits a predominantly elliptical morphology, with a slight elongation that could be indicative of a mild cigar shape. The light distribution is centrally concentrated with a bright core, fading gradually outward towards the edges of the galaxy's visible extent. The overall color appears to be yellowish-red. There is no obvious evidence of spiral arms, dust lanes, or other distinct features within the galaxy's disk. The lack of strong blue emission suggests a relatively low rate of on-going star formation. There is no apparent evidence of any major merger events or significant tidal disturbances.
