This galaxy appears to be undergoing a significant merger event. There are two distinct, luminous components. The primary component exhibits a relatively smooth, elliptical morphology and is characterized by a yellowish hue, suggesting an older stellar population. The secondary component, though also smooth in appearance, is slightly less defined and exhibits a similar yellowish color, possibly indicating a similar stellar population age.

There are signs of tidal disturbances are subtle, but some faint, diffuse extensions are observed. These features may be the result of gravitational interactions between the merging components. A notable amount of disturbance within this galaxy could be an indication of minor merger with another galaxy.

The overall color profile suggests relatively low levels of current star formation within the system, though some may be occuring.
