The galaxy presents a somewhat elliptical morphology. Its light profile appears relatively smooth with a bright central bulge. A faint, disk-like structure may be present although no distinct spiral arms are readily discernible. The galaxy's color is mostly pale blue, which may be due to the presence of hot, young stars, indicating ongoing star formation. There is also a slight irregularity in the overall form, which could suggest a past or ongoing minor interaction or disturbance of some kind.
