The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. It appears largely featureless, lacking any distinct spiral arm structures or obvious dust lanes. There is some indication of a slight extension, suggesting it might not be perfectly spherical but leaning towards an oblate spheroidal shape. The galaxy exhibits a strong central concentration of light that gradually decreases outward from the core, indicating a relatively old stellar population and minimal ongoing star formation. The galaxy's light output is generally redder in the central region, which may be due to the higher concentration of older, redder stars and dust obscuration in that area. The outer regions show a more subtle, greenish tinge. There's no compelling evidence of major mergers or strong tidal disturbances, although the galaxy's shape indicates minor asymmetries that could be the result of past interactions or minor mergers.
