The galaxy presents a complex morphology, exhibiting signs of interaction or recent merger activity. The overall structure appears disturbed, with a prominent disk component tilted relative to the line of sight. Spiral arm features are discernible, appearing somewhat flocculent and loosely wound. The color gradient suggests active star formation regions within the arms, indicated by bluer hues, contrasted against a more pronounced reddish bulge. The central bulge region seems moderately sized in comparison to the disk. There is a significant asymmetry in the light distribution, with one side appearing more extended and possibly disrupted, indicating a major gravitational disturbance. A secondary, smaller luminous knot is visible nearby, hinting at a possible merging companion or a tidal feature resulting from past interaction.
