The galaxy presents as an elliptical-like system. It exhibits a centrally concentrated light profile that gradually decreases in intensity outwards, suggesting an older stellar population dominating the core. The galaxy appears relatively smooth in texture, without prominent spiral arm structures or significant dust lanes, which aligns with an early-type classification. The color index indicates a subtle reddening, typical for galaxies at its distance with a moderately low ongoing star formation rate. While a slight asymmetry is noted in the outer regions, it does not appear to be undergoing a major merger event; subtle tidal features suggest possible minor interactions in its recent history.
