The galaxy presents as a somewhat diffuse, centrally concentrated object. There is an apparent interaction or merger occurring, with the primary body showing a distorted morphology. The primary component has a yellowish hue suggesting an older stellar population. To the right of the primary component, there appears to be a distinct, bluer region, possibly indicative of more recent star formation triggered by the interaction. A fainter, reddish area is seen to the left, possibly a tidal feature. Overall, the system does not appear to be a well-defined spiral or elliptical galaxy, and exhibits evidence of significant dynamical disturbance.
