The galaxy presents a centrally concentrated morphology with a bright, unresolved core. Diffuse light extends outwards from the core in a roughly elliptical shape, although irregularities suggest a potential deviation from a perfectly smooth structure. There are some subtle features that could be indicative of minor disturbances or ongoing interactions, though a definitive classification is difficult at this resolution. Overall, the galaxy exhibits a fairly regular structure, with a degree of central concentration, and is relatively isolated in this field of view.
