The galaxy exhibits a centrally concentrated morphology with a bright nucleus surrounded by a more diffuse, elongated disk. The central bulge appears roughly spherical and dominates the overall luminosity. Evident is a slight asymmetry in the outer regions of the disk, suggesting a possible gravitational disturbance. Faint tidal features may be present, indicating a potential minor interaction with another galaxy, past or ongoing, although this is uncertain. Color variations are subtle, with the central bulge showing a slightly bluer hue compared to the disk, perhaps indicative of recent or continued star formation in the nuclear region. The disk appears relatively smooth with only subtle features. Overall, this galaxy presents characteristics consistent with a disk galaxy undergoing some form of minor interaction or disturbance. Further spectroscopic analysis would be beneficial to confirm potential tidal features and determine the star formation rates in different regions of the galaxy.
