The galaxy appears as a moderately bright, somewhat elliptical object. Its central region exhibits a concentrated, yellowish hue, suggesting an older stellar population. The outer regions display a bluer tint, potentially indicative of ongoing or recent star formation activity. While no distinct spiral arm structures are clearly visible, there may be some subtle features or a disk-like component present within the overall galactic structure. There is a potential indication of a minor gravitational disturbance event occurring. The overall morphology suggests an intermediate stage of galaxy evolution.
