The galaxy presents as a relatively compact object with a smooth, diffuse morphology. There is a slight elongation, suggesting it is not perfectly spherical. The central region exhibits a brighter, more concentrated luminosity, possibly indicating a higher stellar density or an active galactic nucleus. The color appears somewhat blue, potentially signifying a population of younger, hotter stars. No distinct spiral arms or prominent dust lanes are discernible. There is no apparent interaction or major disturbance with nearby galaxies. The overall impression is that of a relatively undisturbed galaxy that is in between round and cigar shaped.
