The galaxy presents an elongated morphology, appearing as a diffuse, roughly elliptical structure on the sky. Its light profile appears relatively smooth, with a gradual decline in intensity from the central region outwards. A slight bluing in color is observed, particularly towards what might be considered the center of the galaxy. The smoothness suggests a possible elliptical classification, but the slight bluing and disk-like appearance suggest some star formation is taking place. Some indication of disturbance or merging is present, possibly in the form of an uneven structure or distortion of its overall shape. This could be the result of a past or ongoing interaction with another galaxy.
