The galaxy presents as a somewhat diffuse object with a central condensation that is slightly brighter. The overall structure appears disturbed or irregular, as it lacks a clearly defined spiral or elliptical morphology. The light distribution suggests the possibility of tidal features or ongoing interactions, with some asymmetric extensions apparent. Patches of bluer light may indicate regions of more recent star formation. Dust lanes are not clearly visible, but cannot be ruled out given the limited image quality. The galaxy appears relatively compact within this field of view. The edges of the object fade into background.
