The galaxy presents as a relatively smooth, though not perfectly elliptical, structure. It appears as an intermediate-type galaxy, positioned somewhere on the continuum between elliptical and spiral morphologies. There is a suggestion of faint, diffuse disk features; however, these are not pronounced.

The galaxy displays a discernible color gradient, with the central regions appearing slightly redder than the outer regions. This may suggest an older stellar population concentrated towards the center. Overall, the galaxy possesses a moderate degree of central concentration. There is no evidence of any significant ongoing merger activity or major tidal disturbances.
