This galaxy presents as a relatively bright, centrally concentrated object, exhibiting a smooth and mostly round morphology. The color gradient suggests a redder core region, potentially indicating an older stellar population or increased dust obscuration towards the center. A fainter, similarly elongated structure is visibly connected to the main galaxy. This secondary component seems to be exhibiting signs of tidal disturbance or interaction, possibly a smaller galaxy being gravitationally disrupted or a tidal tail. There might be evidence of weak tidal features surrounding this galaxy, like an extended envelope or faint streams. The overall appearance suggests a system undergoing or having recently undergone a minor merger event.
