The observed galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, with a gradual decrease in luminosity moving outwards. The overall shape is somewhat elongated, appearing more "in-between" elliptical and cigar-shaped, but without any distinct spiral arm features. The galaxy displays a relatively uniform color distribution, with a slight reddening towards the central region, suggesting an older stellar population in the core. The overall appearance suggests that this galaxy is likely an elliptical, with a dominant bulge and smooth luminosity profile. There is no evidence of any recent or ongoing major merging events; the object seems relatively undisturbed. Evidence indicates star formation is occuring, however, it is likely not the defining characteristic.
