The galaxy presents as a singular, largely featureless object. It exhibits a high degree of radial symmetry with a mostly smooth light distribution. The galaxy displays a notable concentration of luminosity towards the center, suggesting a prominent galactic nucleus. The overall shape appears to be spheroidal, approaching a circular form when viewed from our perspective. The color profile suggests a spectral energy distribution that is brighter in the redder bands, possibly indicating an older stellar population with a suppressed rate of star formation. No clear evidence of spiral arms or a distinct disk component is discernible. There is no strong indication of tidal disturbances or ongoing mergers. The galaxy appears relatively isolated, without obvious companion galaxies or significant gravitational interactions.
