The galaxy presents as a moderately bright, elliptical structure with a concentrated central bulge. It exhibits a relatively smooth morphology, lacking prominent spiral arms or distinct features. The light distribution suggests a gradual decrease in brightness from the core outwards, indicating a well-established stellar population. The galaxy appears elongated, but not to an extreme degree, with the major axis significantly longer than the minor axis. The color gradient suggests a potentially older stellar population dominating, as the core has a yellow hue. A slight disturbance is also noticeable on the outer edges of the galaxy, which might be from a small collision.
