The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. The overall color is yellowish-orange, suggesting an older stellar population with lower rates of on-going star formation. The apparent roundness of the galaxy indicates a possible E0-E3 classification on the Hubble sequence. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed with no major signs of merging events. A slight elongation is observed, suggesting a departure from perfect spherical symmetry.