The galaxy presents as a cigar-shaped, relatively smooth system. The light distribution appears centrally concentrated, with a noticeable elongation along its major axis. The color appears bluer toward the central region, transitioning to redder hues in the fainter outer regions of the galaxy. There is no clear evidence of prominent spiral arms or a distinct disk structure. The galaxy appears to have a relatively small angular size, with a diffuse edge, suggesting a gradual decline in stellar density outwards from the center. It shows no signs of any major disturbances.
