The galaxy presents as a somewhat smooth, elliptical structure with a concentrated central bulge. The light distribution suggests a spheroid-dominated system. The main body is extended and slightly elongated, appearing more "in-between" round and cigar-shaped. The core exhibits a brighter, yellower hue, potentially indicating an older stellar population. Fainter, bluer arms or extended disks are not obvious, further suggesting an earlier-type morphology. There's no visible evidence of major mergers or strong tidal interactions. A subtle disturbance is suspected. Overall, the galaxy appears largely undisturbed.
