The galaxy appears to be a spiral galaxy, though its features are somewhat diffuse. The central bulge is prominent, exhibiting a bright, concentrated luminosity. Surrounding the bulge, the disk is less well-defined, with a more irregular structure. Faint spiral arms appear to emanate from the core, hinted at by subtle variations in color and brightness across the galaxy. The overall color suggests a mixture of stellar populations; the central bulge and parts of the disk appear more yellow/white, potentially indicating older stars, while the spiral arms have a bluer tint, possibly signaling ongoing star formation. There is some indication of disturbance, which may possibly be caused by a merger. The object exhibits intermediate roundness, and it isn't strongly elongated. Overall, the galaxy presents characteristics suggesting a mature spiral galaxy with potential ongoing star formation, and the shape of the galaxy is not highly asymmetrical or disturbed, but does not appear to be perfectly smooth. 
