The galaxy appears to be a relatively compact, early-type galaxy, likely an elliptical or lenticular galaxy. It presents a generally smooth morphology, with a notable concentration of light towards its center, indicating a prominent galactic bulge. There is a slight elongation in its overall shape, more cigar shaped than round. There is little evidence of spiral arms or significant disk features within the observed portion of the galaxy. The color suggests a relatively old stellar population, as it is more concentrated in redder wavelengths. There's a subtle suggestion of minor structural disturbance, possibly due to a past interaction or merger, though the primary structure remains largely undisturbed. The object displays a moderate degree of star formation, but not at an extremely high rate. Its absolute magnitude suggests it is a fairly luminous object.