The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The light profile appears centrally concentrated with a gradual decrease in intensity towards the outer regions. A slight elongation is observed, deviating somewhat from a perfectly circular morphology. There is some indication of a diffuse halo surrounding the main body of the galaxy, though the signal-to-noise is not high enough to resolve any distinct structures within it. The color index indicates a relatively red population, suggestive of an older stellar population and a low ongoing star formation rate. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears to be relatively isolated with some evidence of a smaller nearby object possibly in proximity. Overall, the galaxy is likely a massive, evolved system with a high degree of radial symmetry and minimal ongoing star formation.
