The galaxy presents as a generally smooth object, with a slight elliptical morphology. The core region exhibits a concentrated, bright, yellow-white hue, suggesting an older stellar population or significant dust obscuration. Moving outward from the core, the color transitions to a bluer shade, indicating the presence of younger stars or a less obscured view of stellar populations in these regions. Irregularities in the outer regions suggest the possibility of minor disturbances or interactions. There is a notable absence of clearly defined spiral arms or a distinct disk structure in the image. Based on the colors in the image, this galaxy has an active star formation rate, and would be classified as a massive galaxy.
