This galaxy presents an elongated, cigar-shaped morphology. The central region appears brighter and exhibits a yellowish hue, suggesting an older stellar population likely concentrated in a bulge. Proceeding outwards along the major axis, the color shifts towards a bluer tone. This suggests the presence of younger, hotter stars and active star formation regions in what may be a disk component, but without a clear spiral structure. There are no prominent dust lanes or other distinct features visible within the image. The smooth and somewhat diffuse appearance hints that this may be an elliptical galaxy with some disk-like qualities. A portion of the light emitted from this galaxy has been redshifted, indicating it is receding from us due to the expansion of the universe.
