The galaxy presents as a roughly elliptical structure, with a noticeable bulge region appearing concentrated toward the center. The color distribution suggests a radial gradient, with the central bulge exhibiting a pinkish hue, possibly indicative of an older stellar population. The outer regions are bluer, hinting at ongoing or recent star formation within a disk-like component. Overall, the galaxy is rather smooth in appearance with only a few minor disturbances. The galaxy does not appear to be perfectly circular, but rather slightly elongated, hinting at a flattened spheroidal shape. There are some possible signs of minor interactions occurring, and it would benefit from higher-resolution imaging.