The galaxy exhibits a morphology that appears largely smooth, with a significant fraction of its light concentrated in a central bulge. It presents a roughly elliptical shape, showing a moderate degree of roundness, with a hint of elongation. There is a visible colour gradient, transitioning from bluer hues in the surrounding area to redder tones near the core. This may indicate a difference in stellar populations, with older, redder stars dominating the central region, and younger, bluer stars in the outer regions. Based on its appearance, the galaxy may show signs of possible tidal disturbances or a recent merger event, though it is difficult to say with certainty.
