The galaxy presents a primarily smooth morphology. There is a dominant central region that appears nearly spheroidal. Evidence of a faint disk can be seen, indicating a small degree of internal structure. Its elliptical shape displays a high concentration of light. There may be a potential minor disturbance, but it is difficult to determine based on the image alone. The galaxy exhibits a blue hue, especially within the central core, suggesting the presence of relatively young stars or active star formation. The colors of the arms tend toward redder wavelengths, which is expected for older star populations.
