The galaxy presents as a largely elliptical system, exhibiting a smooth, concentrated central bulge. The overall color profile is dominated by redder wavelengths, suggesting an older stellar population. There is a degree of asymmetry or possible disturbance in the galaxy's morphology, indicative of a potential past or ongoing interaction. It is possible that the galaxy is in the midst of a merger event, which is suggested by a merging fraction of 0.37. The galaxy appears quite massive and exhibits a low star formation rate.
