The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated luminosity distribution with no readily apparent spiral arms or bar structures. Its overall color is indicative of a moderate to old stellar population, exhibiting a subtle blue hue in its central region. The isophotes are generally regular, with only slight deviations from perfect ellipticity, showing a minor disturbance or asymmetry in the outer regions. The galaxy is relatively compact, estimated to be approximately 3 kiloparsecs in radius. There are no obvious signs of a major ongoing merger, although minor tidal features or interactions cannot be entirely ruled out. Overall, this appears to be a relatively undisturbed galaxy that is likely to be actively forming stars.
