The galaxy presents as a somewhat diffuse object with a central, brightened region. The overall morphology appears generally smooth, though with some irregularities present. There appears to be a slight elongation with light spread in the Northwest direction. There are hints of potential disturbance or merging activity within the galaxy's structure. The light distribution across the galaxy is not uniform; the central region exhibits a brighter, possibly active galactic nucleus or a concentration of stars. This object is neither uniformly circular nor extremely elongated, appearing in between. The color gradients suggest a varying stellar population, with bluer regions indicating younger stars and possibly ongoing star formation, and a hint of redder regions indicating older, cooler stars. Based on this morphology, a classification as an early-type spiral or lenticular galaxy could be considered. Further spectral analysis would be needed to confirm the star formation rates and dynamics within the galaxy.
