The galaxy presents as a relatively smooth, rounded structure, exhibiting a notable concentration of light towards its central region. A faint, diffuse halo appears to extend outwards from the core, suggesting a gradual decrease in stellar density with increasing radial distance. There is a subtle indication of a disk-like structure, though it is not clearly defined. The overall color appears to be skewed toward the redder end of the spectrum, indicative of an older stellar population. There is no immediately apparent evidence of ongoing major mergers or significant tidal disturbances, although a subtle asymmetry or minor disturbance cannot be entirely ruled out. The galaxy appears largely undisturbed with no significant dust lanes or regions of intense star formation visible in this image.
