The galaxy presents a generally smooth morphology, with a notable lack of distinct spiral arms or a well-defined disk structure. The overall shape is elongated, tending towards an intermediate elliptical form rather than a perfect sphere. The central region exhibits a higher surface brightness, suggesting a concentration of stellar mass or active galactic nucleus activity. The color profile appears relatively uniform across the galaxy, with a yellowish-orange hue indicative of an older stellar population. There are subtle hints of a very small amount of blue star formation in the outer regions, but the galaxy is dominated by older, redder stars. No strong signs of tidal disturbances or major mergers are readily apparent, although some minor asymmetries in the outer isophotes cannot be ruled out.
