The galaxy presents as a singular, largely featureless object. Its morphology appears primarily elliptical, exhibiting a high degree of sphericity. The central region presents a concentrated luminosity gradient, suggesting a significant stellar population density. Colors across the galaxy appear relatively homogenous, with a general trend toward yellow, indicating an older stellar population with reduced star formation. There is no evidence of spiral arms or prominent dust lanes. The overall shape is relatively smooth and undisturbed, suggesting a lack of recent major mergers or significant interactions.
