The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile suggests an older stellar population, exhibiting a redder hue. The galaxy demonstrates a general lack of strong spiral arm features or significant dust lanes, indicating it is likely a passively evolving system. There is a hint of some interaction or minor disturbance, but overall the galaxy appears to be relatively undisturbed, and exhibits characteristics indicating the absence of a recent major merger event. The galaxy appears to be luminous. The object demonstrates a high degree of roundness with slight indications of being in between round and cigar-shaped, which also suggests the likelihood of it being an elliptical galaxy.
