The galaxy presents a generally smooth morphology, with an ovoid shape. The central region exhibits a concentrated luminosity with a yellow-orange hue. Proceeding outward from the center, the luminosity decreases, and the color profile shifts towards a bluer tint. This may indicate a population of younger stars forming outside the galactic nucleus. There's no clear evidence of spiral arm structure or a prominent disk. The overall appearance suggests it is an elliptical or lenticular galaxy, with a moderately high estimated stellar mass and a low but present rate of star formation. There is a very slight chance of minor tidal disturbances, but overall it has a relaxed undisturbed morphology.
