The galaxy presents as a slightly elongated, diffuse object with a discernible central bulge. The bulge exhibits a yellowish-orange hue, suggesting a population of older stars. Extending outwards from the bulge, a faint, bluish disk can be observed, indicating the presence of younger, hotter stars and potentially ongoing star formation. The galaxy appears to be relatively smooth in overall structure, although there are subtle irregularities in the disk. One side seems a bit disturbed, with a smaller, blueish area close to the disk, which suggests this galaxy may be undergoing a minor disturbance or interaction. Overall, this appears to be a disk-type galaxy with a prominent bulge, viewed at an oblique angle. The color gradients suggest a mix of stellar populations and evolutionary stages.
