The galaxy presents as a centrally concentrated elliptical or lenticular system, exhibiting a smooth, diffuse morphology. There is a high degree of symmetry around the central bulge, with a gradual decrease in luminosity from the core outwards. The galaxy appears flattened, with a relatively high ellipticity.

The color profile suggests an older stellar population, with a dominance of redder wavelengths, particularly in the central regions. Fainter, bluer light can be seen further out from the central concentration. There is no evidence of spiral arms or significant dust lanes within the visible spectrum. The galaxy appears undisturbed, with no obvious signs of tidal interactions or recent merger events.
