The galaxy presents a generally smooth, centrally concentrated morphology. It exhibits a slight degree of asymmetry, possibly suggestive of a minor interaction or internal disturbance. Its ellipticity is low, trending towards round, with a subtle elongation. The color profile shows a general blueness overall, with the central region being more strongly blue-shifted. This suggests the presence of a younger stellar population. There is no strong evidence of spiral arm structure, bar structure, or a distinct nucleus. The overall appearance is consistent with a lenticular or early-type spiral galaxy, transitioning towards an elliptical shape.
