The galaxy presents as a relatively smooth object, exhibiting characteristics consistent with an elliptical morphology. The light is concentrated toward the center, indicating a prominent nucleus, and decreases smoothly and steadily outward. There is no strong indication of any spiral arm structure.

The light distribution suggests a moderately spheroidal shape. The color appears to be a somewhat blue, possibly indicating some degree of recent star formation. The absence of prominent dust lanes or features typically associated with ongoing mergers suggests that this galaxy is relatively settled, and that the star formation is likely proceeding at a modest rate. There is no obvious indication of interactions with neighboring galaxies, or other significant perturbations of its structure. The outer regions of the galaxy fade gently into the background sky, indicating that the galaxy is reasonably well defined.

