The galaxy presents as a moderately elliptical structure, appearing somewhat smooth with a bright central bulge. The outer regions display a more diffuse glow, suggesting the presence of a galactic disk, though without prominent spiral arm features visible at this resolution. There is a subtle color gradient observable, with a slightly bluer hue apparent in the outer regions compared to the redder central bulge. The galaxy lacks any obvious signs of ongoing major mergers or significant tidal distortions, although the faint irregular light distribution hints at minor disturbances or interactions in its past. Overall the galaxy appears to be relatively well-defined, lacking strong evidence of active starburst activity, though some star formation is likely still occurring.
