The galaxy presents a relatively smooth, though not perfectly spherical, morphology. Its light distribution appears centrally concentrated. There are hints of possible faint, diffuse extensions or a very faint, broad disk, but the limited resolution makes this uncertain. The galaxy exhibits a blue hue, suggesting the presence of a younger stellar population and ongoing star formation, although it is not highly active. There is evidence of some disturbance, potentially from a minor interaction or a small-scale merger. The galaxy doesn't show any strong signs of spiral arms or a well-defined bar structure.
