The galaxy presents a generally smooth, elliptical morphology. It appears somewhat rounded, with a gradual falloff in luminosity from the core outwards. There is no strong evidence of spiral arm structure. The central bulge is prominent, exhibiting a higher surface brightness than the surrounding halo. Faint, diffuse features are subtly present, suggesting possible minor disturbances or interactions. The overall color is consistent with an older stellar population, presenting a reddish hue.
