This galaxy appears to be an elliptical type, displaying a generally smooth and featureless morphology. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The luminosity appears to gradually decrease with increasing radial distance from the center. There is some asymmetry in the outer regions, which could indicate minor disturbances and hints of past or ongoing interactions. A faint, diffuse halo surrounds the main body of the galaxy, visible as a gradual fading of light. The color of the galaxy appears slightly redder in the central bulge, with bluer hints in the outer regions. This is suggestive of an older stellar population in the center and younger stars present in the surrounding regions. The object does not present any obvious spiral arm structures.
