The galaxy presents as a relatively smooth, elongated structure. Its color profile appears to shift from a central yellowish-white hue to a more reddish outer region. The galaxy exhibits an elliptical morphology, displaying a cigar-like shape. There is no apparent evidence of a substantial merger or significant tidal disturbance. The overall light distribution is relatively concentrated, indicating a potential high stellar mass. Given the redder color on the outskirts and lack of blue star-forming regions, star formation may be limited.
