This galaxy exhibits a moderately bright central bulge that appears relatively smooth and concentrated. The surrounding disk shows distinct features, with an apparent irregular shape. The color gradients suggest variations in stellar populations, with a concentration of bluer light potentially indicating regions of active star formation within the disk and around the bulge. There appears to be some asymmetrical distribution of luminosity suggesting possible tidal interactions, although a classic spiral arm structure is not obviously apparent. The overall morphology leans toward a spiral type with some level of disturbance.
