The galaxy presents as a primarily smooth structure, exhibiting a notable elongation. Its overall shape is reminiscent of a cigar, being significantly longer than it is wide. The core region appears relatively bright and concentrated, with a yellowish hue suggesting an older stellar population. The outer regions of the galaxy fade into the background, and may consist of a faint disk. There is no evidence of major disturbances or ongoing mergers in the visible morphology. The overall color suggests a galaxy where star formation may be suppressed.
