The galaxy presents as a single, relatively smooth object with a centrally concentrated luminosity profile. It appears elliptical in shape, displaying a high degree of radial symmetry. The core is luminous, exhibiting a yellow-orange hue that transitions into a slightly redder periphery. There is no distinct spiral structure, bar, or other evident morphological features indicative of recent mergers or strong tidal interactions. The galaxy's color suggests an older stellar population with minimal ongoing star formation. Overall, the object appears to be a fairly massive, early-type galaxy.
