The galaxy presents as a single, relatively smooth object, with minimal visible substructure. It exhibits a centrally concentrated luminosity profile, appearing nearly round. Color gradients across the galaxy are subtle, with a slightly redder hue towards the center. This suggests an older stellar population dominates the core region, or a presence of dust. Overall, the galaxy seems to be relatively undisturbed. There is no evidence of tidal tails or significant morphological disturbances indicative of recent major mergers. Faint hints of bluer color along the edges may indicate ongoing low levels of star formation in the disk.
