The galaxy presents as a centrally concentrated object, roughly elliptical in shape, with a bright, somewhat disturbed core. The central region displays a marked bluish hue, suggestive of ongoing star formation. Moving outward from the center, the color transitions to a more reddish or yellowish tone, indicative of an older stellar population. The galaxy's overall structure appears smooth, though the central region shows some asymmetry and possible features of a disk. There is faint evidence of minor disturbances or tidal features extending from the main body of the galaxy. The object's morphology is likely somewhere between an elliptical and a spiral galaxy. The estimated distance places the object at a considerable redshift, given the apparent magnitude.
