The galaxy presents a generally elliptical morphology, with a smooth, concentrated central bulge exhibiting a yellowish-white hue, indicative of an older stellar population. A fainter disk-like structure surrounds the bulge, extending outwards and displaying hints of spiral arms. These arms show patches of bluer colors, possibly regions of active star formation. There is some disruption in the symmetry of these spiral arms indicating potentially minor disturbances that could be due to ongoing or recent mergers. The outer regions fade into the background, suggesting a low surface brightness. Overall the object does not exhibit a well-defined spiral structure, and presents as somewhere between a spiral and elliptical type. The galaxy is observed at a redshift of z=0.24, indicating a significant distance.
