The galaxy presents as an elongated, elliptical structure with a smooth, diffuse appearance. It appears relatively featureless, lacking prominent spiral arms or dust lanes that would indicate significant ongoing star formation within a disk component. The light distribution is concentrated towards the center, suggesting a central bulge, and fades gradually towards the outer edges. The galaxy exhibits a color gradient, with the central region appearing bluer, possibly indicating a younger stellar population. This bluer light suggests more star formation than the more dim regions, which appear slightly redder, potentially indicating an older stellar population dominated by redder stars. The overall morphology suggests the galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy nearing the end of its evolution. There is some indication of a possible minor tidal disturbance or interaction in the galaxy's halo.
