The galaxy presents a morphology that suggests a relatively smooth structure with some indication of a disk feature. The central region appears as a bright, concentrated bulge exhibiting a yellowish hue, likely indicative of an older stellar population. Surrounding the bulge is a fainter, bluer halo. There is a slight asymmetry or some mild disturbance in the disk, but it is primarily undisturbed. This galaxy is likely not in the midst of a major merging event but may have had a minor interaction in its past. The overall color profile and smooth appearance could suggest a galaxy in a transitional phase, between a more actively star-forming state and a quiescent one.
