The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation along its major axis. The central bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Fainter, bluer regions extend outwards from the core along the equatorial plane, potentially indicative of some level of ongoing star formation within a disk-like structure. There are no obvious signs of strong spiral arms or a bar structure. A subtle degree of asymmetry may be present in the outer regions, but further analysis is required to determine if it is intrinsic to the galaxy or a result of tidal interactions. There's no evidence of a major merger event, with possible signs of a minor disturbance. Overall, the galaxy appears to be an intermediate-mass system at a moderate redshift, exhibiting characteristics of a galaxy transitioning away from active star formation.
