This galaxy exhibits a somewhat elongated morphology. The central region presents a brighter, more concentrated luminosity profile. Moving outward from the core, the light becomes progressively fainter. There is evidence of a faint disk-like structure with some possible indications of spiral arm features. The light from the disk appears slightly bluer than the central bulge. The galaxy may be undergoing some sort of interaction, given its asymmetry. It is neither perfectly elliptical nor a well-defined spiral. The overall appearance suggests a galaxy that may be in transition or has experienced recent gravitational disturbances.
