This galaxy presents as a relatively smooth, elliptical form. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The galaxy transitions to a greenish hue towards its outer edges, potentially indicating the presence of younger, hotter stars or ionized gas. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy has an elongated shape, with the major axis significantly longer than the minor axis, appearing cigar-shaped. There are no signs of major mergers or tidal disturbances, though there might be some minor asymmetry, suggesting a possible past interaction or minor disturbance. Overall, the galaxy appears to be a fairly evolved system, with a dominant older population and a moderate level of on-going star formation in its outskirts.
