The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification. The light profile appears centrally concentrated with a gradual decrease in intensity outwards. The shape is largely in between round and cigar-shaped, although tending towards a slightly elliptical appearance rather than perfectly spherical. There is no clear evidence of spiral arms, a distinct disk, or a central bar structure. The galaxy exhibits a yellow-white color, potentially indicating an older stellar population with fewer young, massive stars. Minor disturbances may be present. There does not appear to be a ongoing major merger. Overall the galaxy looks reasonably undisturbed.
