The galaxy presents an elongated, cigar-shaped morphology. Its light is dominated by a smooth, featureless central bulge, with a noticeable color gradient from the center outwards. The core exhibits a concentration of light with a slightly redder hue, which may indicate an older stellar population. The outer regions of the galaxy have a bluer tint, potentially suggesting more recent star formation activity. Some minor disturbances appear present in the galactic structure, specifically some areas with slight distortions. It seems to be potentially undergoing a merger event. Overall, the galaxy's light is evenly distributed, with no distinct spiral arm features visible in this imagery.
