The galaxy appears to be a relatively compact object, exhibiting a largely elliptical morphology. The central region presents a higher concentration of light, suggesting a prominent bulge. The overall color profile indicates a population of stars with a mix of ages, where the bulge exhibits a greater concentration of older, redder stars, while the outer regions possess a bluer hue, hinting at ongoing or recent star formation. There may be some faint signs of tidal disturbances. There is a small asymmetry in the outer structure, possibly indicating a minor interaction. The galaxy shows a degree of smoothness in its light distribution, lacking any prominent spiral arms or other complex structures.
