The galaxy presents as a smooth, elliptical morphology. The central bulge is prominent and appears relatively bright, suggesting a higher concentration of older stars. The overall color is yellowish-red, indicative of a relatively old stellar population with little ongoing star formation. The galaxy is somewhat elongated in shape, and displays a smooth light distribution, without any visible spiral arms or strong dust lanes. There is a faint, extended halo surrounding the central region, indicating the presence of a diffuse stellar component. There is no evidence of significant tidal disturbances or ongoing mergers.
