The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal, with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the light gradually diffuses into a slightly reddish halo. This halo region appears to be composed primarily of low surface brightness light, with hints of older stars and very little dust obscuration. There is no strong evidence of spiral arm structure or a well-defined disk. Some faint, diffuse light extends from the main body of the galaxy, giving it an estimated effective radius on the order of several kiloparsecs. No significant signs of ongoing merging activity, major tidal disturbances, or a prominent active galactic nucleus are immediately apparent in the image.
