The galaxy presents as a moderately luminous, elliptical structure, exhibiting a smooth, featureless morphology. The central region displays a higher concentration of luminosity, suggesting the presence of a prominent galactic nucleus. A subtle color gradient is apparent, with a shift towards redder hues observed in the central region. This may indicate an older stellar population is located at the center of the galaxy. The isophotes appear somewhat elongated, deviating slightly from a perfect circular shape. There is no visible evidence of spiral arms, dust lanes, or other distinguishing features typically associated with spiral or irregular galaxies. Overall, the galaxy seems relatively undisturbed, showing no signs of major mergers or tidal interactions.
