The galaxy presents as a moderately bright, elliptical-shaped structure. Its core is luminous and concentrated, exhibiting a smooth, diffused glow. Proceeding outward from the core, the galaxy's light gradually diminishes, lacking prominent spiral arms or distinct features. There is a possible minor disturbance or companion galaxy nearby, with some disruption to the symmetry of the primary galaxy on one side. The overall color appears to be on the redder end of the spectrum, suggesting an older stellar population with less ongoing star formation. The shape leans towards a more oblate spheroid, rather than a highly elongated or spherical form.
