The galaxy presents as a system of two distinct, interacting components. The primary component exhibits a smooth, elliptical morphology, with a concentrated central bulge. Its color is predominantly yellow/gold, suggesting an older stellar population and a lack of significant ongoing star formation.

The secondary component displays a more irregular shape and a bluer color, indicative of younger, hotter stars and possible ongoing star formation activity. This component appears to be interacting with the primary galaxy, with a visible tidal distortion or bridge of material connecting the two. The overall appearance suggests a galaxy merger in progress, possibly a major or minor merger depending on the relative masses of the two components. Faint wisps or tails are suggestive of gravitational interactions or tidal forces at play. The tidal features are subtle, indicating that this system is not undergoing a recent violent merger.
