The galaxy presents as a relatively smooth, elliptical object. The central region exhibits a brighter, concentrated luminosity, suggestive of a prominent galactic nucleus. The radial light profile appears to decline smoothly outward from the center. Overall the galaxy has a goldish hue, slightly brighter in its core. Faint extensions are visible along what appears to be its major axis. These extensions do not seem to form distinct spiral arms. The galaxy appears largely undisturbed, with no apparent signs of ongoing major merger activity, however, some possible signs of minor disturbances could exist.
