The galaxy presents a somewhat amorphous morphology, with evidence of a possible ongoing or recent interaction or merger event. The primary body of the galaxy exhibits a generally smooth, centrally concentrated luminosity profile. A distinct, though less luminous, secondary component is observed, separated from the primary body by a narrow gap. The color distribution suggests a slightly bluer population within the primary body, possibly indicative of ongoing star formation. Overall, the galaxy appears moderately disturbed and possibly undergoing tidal interactions or a merger with a smaller companion.
