The galaxy presents as a relatively large, elliptical morphology with a smooth, diffuse light distribution. The light appears yellowish indicating an older stellar population dominating its composition. It lacks any prominent spiral arms or distinct dust lanes, further supporting its elliptical classification. The galaxy is relatively bright, suggesting a significant stellar mass and is observed with a mild elongation. There appears to be little evidence of ongoing star formation or recent merger events in this system. The galaxy appears as a well-defined and relatively isolated object within its observed field.
