The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The galaxy exhibits a color gradient, appearing generally reddish-gold in the core, which gradually fades to a more diffuse, yellowish halo. There is very little evidence of spiral arm structure, and the overall morphology suggests a gravitationally relaxed system. The galaxy's light distribution is centrally concentrated, hinting at a high stellar mass concentration within the nucleus. There are no obvious signs of active star formation or dust lanes, suggesting a predominantly older stellar population. The overall impression is that of a mature galaxy. The galaxy appears relatively isolated with no apparent major tidal disturbances.
