The galaxy appears to be relatively compact. It exhibits a generally smooth morphology, with a central region displaying a higher concentration of light. The light is somewhat diffuse, with a slight elongation in its overall shape. There is a faint hint of disturbance or asymmetry within the galactic structure, possibly indicative of minor tidal interactions or internal dynamic processes. Color analysis indicates that the core of the galaxy shows yellow and green hues, potentially indicative of a mix of stellar populations. The outer regions fade into a bluer color, indicating some degree of ongoing star formation. Overall, the galaxy does not show prominent spiral arms or a well-defined disk-like structure.
