The galaxy presents a smooth, elliptical morphology. It exhibits a relatively concentrated central bulge that gradually fades into the outer regions. There is a slight elongation to its shape, appearing somewhat cigar-shaped rather than perfectly spherical. No distinct spiral arms or prominent dust lanes are discernible within the galaxy's structure. The light distribution suggests a relatively old stellar population, consistent with a low star formation rate. There is no noticeable interaction with other galaxies or signs of recent major mergers, indicating a dynamically stable system.
