The galaxy presents a complex morphology, appearing neither purely elliptical nor possessing a well-defined spiral structure. The light distribution is concentrated toward the center, displaying a degree of smoothness suggestive of an early-type galaxy influence. However, faint and subtle features hint at the possibility of a disk component or tidal disturbances. There appears to be a possible faint merging companion or tidal tail extending outward, indicating a recent or ongoing interaction. The color profile suggests a mixture of stellar populations; the core region exhibits a yellow hue, consistent with older stars, while the outer regions display a bluer tint, which might be attributed to younger stars within a disk. The galaxy's overall shape tends towards being oval, but not perfectly spherical. Evidence suggests it is neither currently undergoing a major merger, nor completely undisturbed.
