The galaxy presents as a disturbed system, showing evidence of a possible ongoing or recent merger event. The primary galactic body appears somewhat amorphous, lacking a clearly defined spiral structure or elliptical shape. There is a noticeable blue hue indicating star formation. A distinct red region is visible, suggestive of either a concentration of older stars, obscured dust, or intense activity such as star formation within a dusty environment. The overall light distribution is relatively diffuse, without a highly concentrated central bulge, but the overall shape is mostly smooth with some irregular features.
