The galaxy presents as a relatively smooth, elliptical morphology. It appears largely spheroidal with a noticeable elongation, trending towards a cigar shape. There is a concentration of light towards the center suggesting a prominent galactic bulge. The color is consistent with an older stellar population, exhibiting redder hues throughout. The light is smooth, diffuse, and lacks distinct features such as spiral arms or strong dust lanes. There is no evidence of any ongoing major merger or significant tidal disturbance. Any potential minor disturbance is difficult to ascertain. Overall, the galaxy presents as a settled, evolved system.
