The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge is apparent, with a color gradient indicating a relatively older stellar population dominating the core. Fainter, bluer regions surround the central bulge, suggesting the presence of a younger stellar population and ongoing star formation in the outer regions. There are some features showing minor asymmetrical disturbance of its main structure, possibly due to a minor gravitational interaction. No prominent spiral arms are visible.
