The galaxy presents a primarily smooth morphology, exhibiting characteristics consistent with an elliptical or lenticular type. The light distribution is generally centrally concentrated, fading gradually towards the edges. The shape is moderately elongated, but leans towards an oval appearance rather than a distinctly flattened disk. A slight color gradient is observed, with the central region exhibiting a yellowish to reddish hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, which could imply the presence of younger stars, however, this is only a slight difference. There is also an indication of some disturbance of the light in the structure, but it is not an extreme disturbance. Overall, the galaxy appears relatively isolated, displaying no clear signs of ongoing major interactions or mergers.
