The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a diffuse, elliptical morphology with no distinct spiral arms or bar structure visible. The core region displays a bright, concentrated luminosity, suggesting the presence of a dense stellar population or active galactic nucleus. The galaxy's color is generally yellowish-white, indicating a population of older stars and a lower rate of ongoing star formation. Some subtle mottling and minor irregularities can be observed in the galaxy's outer regions, hinting at possible past interactions or internal dynamics. There appears to be a slight asymmetry to the overall shape, possibly caused by tidal interactions with another galaxy, though no major disturbances are obvious.
