The galaxy presents as a system of gravitationally interacting galaxies. The primary galaxy exhibits a smooth, somewhat elliptical morphology, with a color gradient suggesting a higher concentration of older stellar populations within its core and a slightly bluer periphery. There is evidence of ongoing or recent interaction with a nearby galaxy that lies slightly above the main galaxy. This smaller galaxy appears less defined and more diffuse, possibly indicative of tidal disruption due to the larger galaxy's gravitational influence. The system's overall color profile suggests moderate star formation activity. There are possible faint tidal features emanating from the smaller galaxy, further supporting an ongoing merger event. The system's overall shape appears slightly disturbed, with subtle asymmetries in the light distribution, hinting at past or continuing interactions influencing the galactic structure.
