The galaxy presents as an elongated, possibly disk-shaped, structure with an inclination that obscures detailed morphological features. The central region is characterized by a concentrated, yellowish-orange glow, suggesting an older stellar population or significant dust obscuration. Extending from the central region, there appears to be a fainter, bluish component, possibly indicating regions of more recent star formation. The overall structure appears relatively smooth, with no readily apparent spiral arms or strong irregularities, though the potential disk-like shape is slightly disturbed or warped on one side. There may be some low-level merger activity going on, as the edges of the galaxy seem disturbed.
