The galaxy presents as a relatively smooth, elongated structure with a central bulge that appears brighter and more concentrated. The color profile indicates a yellowish-white core region, suggesting an older stellar population dominating the center. The outer regions exhibit a slightly bluer hue. There is no clear evidence of spiral arms or significant dust lanes within the visible structure. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers, although there may be a minor disturbance given its asymmetry. It is a larger galaxy with a substantial stellar mass. The low star formation rate indicates that it is likely a quiescent galaxy, possibly an early-type spiral or elliptical.
