The galaxy presents a predominantly smooth, elliptical morphology with a notable absence of spiral arm structures. Its overall shape appears to be somewhat in between a perfect circle and a cigar shape. Light distribution suggests a centrally concentrated bulge region that gradually decreases in luminosity towards the outer edges, creating a diffused halo. There are subtle irregularities, suggesting possible interactions with other objects. These include what seems to be minor disturbances in the main body, but the galaxy is most likely in an isolated state. Color gradients are subtle, with a slightly bluer hue in the central region that shifts towards redder tones in the periphery.
