The galaxy presents as a relatively smooth, centrally concentrated object with a slight elongation. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Fainter, diffuse bluish-white light surrounds the core, indicating the presence of a younger, star-forming population, although this component is not dominant. There are no clearly defined spiral arms or a prominent disk structure discernible. The overall morphology suggests a galaxy that could be transitioning from a disk-dominated system toward a more spheroidal or elliptical shape. There is a hint of a minor tidal disturbance, but it is unclear if this galaxy is experiencing a significant interaction with another object.
