The galaxy presents as a somewhat elliptical, yet moderately disk-shaped object with a smooth overall appearance. The galaxy's central region appears brighter and more concentrated. There is a slight color gradient, with the central region tending towards a yellower hue, possibly indicating an older stellar population. Fainter blue regions are observed throughout the disk of the galaxy. The relative smoothness suggests a lack of significant ongoing mergers or major disturbances, although subtle asymmetrical features or faint tidal tails may be present upon closer examination. There are no clearly defined spiral arm structures or prominent dust lanes.