The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears relatively bright and uniformly colored. The galaxy appears fairly symmetric, with a round shape. There is a lack of distinct spiral arms or a well-defined disk structure. The color gradient from the core to the outer regions appears minimal, suggesting a fairly homogenous stellar population. There is no apparent interaction with any other nearby galaxy, nor any evidence of any recent merger activity.
