This galaxy presents as an interacting system, exhibiting clear signs of tidal disruption. The primary galaxy appears relatively smooth but irregular, with a yellowish hue indicating an older stellar population. A secondary, smaller component is visible, also yellowish in color, potentially a dwarf galaxy or a region of enhanced star formation within the distorted structure. A faint tidal tail extends from the main body of the galaxy, indicating a recent or ongoing gravitational interaction. The overall morphology suggests a merging event. There is evidence of internal structure distortion, rather than well defined spiral arms.
