The galaxy presents a generally smooth morphology. It appears elliptical in shape, exhibiting a central bulge that graduates into a more diffuse halo. The color profile suggests an older stellar population, with a prominent yellowish-orange hue dominating the central region, potentially indicating a higher concentration of evolved stars. Faint hints of bluer regions at the outer edges may suggest some ongoing, albeit limited, star formation. There is no apparent spiral structure, and there are no indications of any major mergers or tidal disturbances. The galaxy's light distribution is mostly symmetrical. The shape suggests that it is likely an intermediate galaxy in its evolution and is well on its way to becoming elliptical.
