The galaxy presents as a somewhat elongated, likely elliptical, system with a smooth and diffuse morphology. Its color profile exhibits a central concentration of yellow-orange hues that fade into a pale blue as it extends outwards. This color gradient is typical of older stellar populations residing in the inner regions, with younger, bluer stars populating the outskirts. The galaxy appears to be isolated, showing no signs of tidal disturbances or ongoing mergers with other galaxies. The overall structure is relatively undisturbed, suggesting a period of quiescence. It exhibits a cigar-like shape, indicating a significant ellipticity.
