The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high density of stars and potentially the presence of a supermassive black hole. Moving outward from the core, the luminosity gradually decreases, fading into the surrounding space.

There is a subtle hint of a flattened shape, though the galaxy appears predominantly round. No distinct spiral arms or prominent dust lanes are apparent. The galaxy's color profile transitions from a yellowish-white hue in the core to a slightly bluer tint in the outer regions. This color gradient may be indicative of varying stellar populations, with older, redder stars concentrated in the core and younger, bluer stars populating the outer regions, hinting at ongoing, but low levels of star formation. There is no indication of any major mergers or disturbances in its structure; however, very minor asymmetries cannot be ruled out based on the available image.
