The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. Its overall color appears yellowish-orange, suggesting an older stellar population with minimal ongoing star formation. The galaxy exhibits a roughly circular morphology, with a high degree of central concentration. There is no visible evidence of spiral arms, prominent dust lanes, or any signs of recent merger activity or significant tidal disturbance in its immediate vicinity. The galaxy appears to be a fairly isolated system.
