This galaxy appears to be undergoing a merger or interaction. The primary component presents as a luminous, somewhat spherical bulge, exhibiting a smooth light distribution with a bright, concentrated core. This central region displays a distinct blue-green coloration. Extending from this core is a fainter, elongated feature exhibiting a reddish-orange hue. This extension suggests either a tidal tail resulting from gravitational disruption or the remnant of a smaller galaxy involved in an ongoing merger. There is some visual evidence of a possible dust lane or obscuring material associated with the reddish component. Overall, the galaxy exhibits signs of morphological disturbance, deviating from a simple elliptical or spiral structure.
