The galaxy presents a generally smooth morphology, with a high degree of central concentration. It is nearly circular in shape. The galaxy's light profile appears to decrease monotonically from the center outward, suggesting the absence of strong spiral arm features or a well-defined disk component. There is a possible, albeit subtle, tidal feature or minor disturbance extending from the main body, potentially indicating past or ongoing interaction with a smaller companion. The overall color of the galaxy is slightly blue-green, indicating the presence of a young stellar population.
