The galaxy presents as a somewhat elliptical form, exhibiting a smoothly distributed luminosity profile. The central region is markedly brighter, suggesting a concentration of stellar mass or a possible active galactic nucleus, though the resolution is insufficient to confirm the latter. The galaxy exhibits a blue hue overall. The galaxy does not appear to have any major disturbances from any recent mergers. Faint extensions are present along the major axis, indicative of a disk.
