This galaxy presents a somewhat smooth, elliptical morphology. Its overall shape is not perfectly spherical, exhibiting a moderate elongation. The central bulge appears as a concentrated region of bright, yellowish-white light. The light distribution suggests a dominant population of older stars in the bulge. Fainter, more diffuse light extends outwards from the bulge, indicating the presence of a disk component. Within the disk, there are a few faint and dusty features that suggest the presence of some star formation. There is no apparent central bar structure, nor is there any evidence of active galactic nuclei emission in the core. The galaxy appears relatively isolated.
