The galaxy presents a generally smooth morphology with a slight asymmetry in its structure. Its light profile appears somewhat diffuse, suggesting it may be an early-type spiral or lenticular galaxy. There is indication of weak disk features with faint arm-like structures extending from the central bulge. These may indicate low-level star formation. A slight elongation is observed. There are minor signs of disturbances. The galaxy's color profile suggests it is composed of an older stellar population.
