The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high surface brightness, with a concentrated nucleus indicative of an older stellar population. The overall color appears somewhat redder in the core, suggestive of a population of evolved stars. Moving outward from the center, the light gradually diffuses, indicating a decreasing stellar density. The galaxy appears elongated, with an axial ratio that suggests it is not viewed face-on, but rather at an angle to our line of sight. There is a hint of bluer light in the outer regions, possibly indicating a small amount of ongoing star formation, but no distinct spiral arms or prominent features are immediately apparent. The overall structure points to an evolved system that has likely undergone significant dynamical relaxation. There is no strong evidence of any major ongoing merger activity or strong tidal disturbances in the visible light.
