The galaxy presents as an elliptical-type morphology, appearing largely smooth and relatively featureless. Its light is concentrated towards the center, showing a bright, prominent bulge region. The galaxy exhibits a yellowish hue, possibly indicating an older stellar population with lower rates of current star formation. There is a possible small companion galaxy merging with the larger object, indicated by a minor disturbance in the primary galaxy's shape. There is evidence of a recent or ongoing merger event, with a disturbed morphology but lacking strong tidal tails or obvious merger signatures. The galaxy's profile appears to be in between round and elongated. The system appears relatively compact, exhibiting a small angular size on the sky.