The galaxy presents as a single, concentrated luminous object, with a generally smooth and elliptical morphology. The central region exhibits a high degree of luminosity, appearing intensely bright. There is a slight elongation to the galaxy's shape, deviating marginally from a perfectly circular form. The color profile indicates an older stellar population, trending toward redder wavelengths. No obvious spiral arm structures or significant dust lane obscuration are visually discernible. There is a very slight indication of a possible minor tidal disturbance, possibly a very faint plume, but this is marginal and could easily be an artifact. Overall, the galaxy appears as a relatively undisturbed and evolved system.
