The galaxy presents as a somewhat smooth, elliptical-like object. Its core appears bright and concentrated, exhibiting a yellowish-white hue, indicating a population of older stars. Moving outwards from the core, the galaxy transitions to a more diffuse, bluish color, suggesting the presence of some younger stars. The main structure is relatively symmetric and compact, with the possibility of minor tidal disturbances, or interactions that are slightly disrupting the outer regions, giving it an irregular shape. Based on the colors, there appears to be ongoing star formation in the galaxy but at a low rate. The overall morphology suggests a galaxy that is neither a late stage elliptical nor a spiral, but somewhere in between and potentially transitioning from a spiral to an elliptical.
