The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge that gradually fades into a more diffuse, extended halo. The overall shape appears to be somewhat elliptical, deviating slightly from a perfect circular form. A subtle disk-like structure may be present, but it is not distinctly defined, possibly oriented close to edge-on. The color profile suggests a primarily older stellar population, as indicated by the reddish hue concentrated in the central bulge. A subtle presence of bluer colors in the outer regions indicates ongoing, albeit subdued, star formation. There's no obvious sign of strong tidal interactions or recent major merger events, though some minor disturbances cannot be ruled out.
