The galaxy appears to be undergoing a merger or interaction with another galaxy. There are two distinct, somewhat spheroidal, luminous concentrations of stars. One is brighter and more centrally located within the diffuse galactic halo, while the other is less luminous, and slightly elongated. There is also a noticeable tidal bridge of stars and gas connecting the two luminous components, indicating a gravitational interaction. The galaxy shows an overall yellow/red color, suggesting an older stellar population and lower levels of recent star formation. While no prominent dust lanes are directly visible, the morphology of the galaxy is disturbed, possibly due to ongoing tidal forces. The galaxy appears to be of significant mass, given its absolute magnitude and morphology.