The galaxy presents a generally smooth and rounded morphology. A bright central bulge is evident, exhibiting a concentration of light. Surrounding the bulge, a fainter, more diffuse halo or disk is observable. The color appears relatively uniform throughout the galaxy, although there are subtle variations with hints of bluer regions intermixed with redder tones, perhaps indicating some level of ongoing or recent star formation. There is no readily apparent evidence of spiral arms or other distinct structural features within the disk. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
