The observed galaxy presents as a relatively compact object with a smooth, diffuse morphology. The central region appears brighter, suggesting a concentration of older stars or a potential active galactic nucleus, though its smooth appearance argues against the latter. There is a general lack of spiral arm structures or prominent dust lanes. The overall shape is generally round, with no significant elongation or tidal features visible, indicating a relaxed system that may be an elliptical or lenticular galaxy. Color gradients appear minimal, suggesting a relatively uniform stellar population throughout the galaxy. There is no obvious evidence of on-going major mergers or significant star formation activity.