The galaxy presents as a somewhat diffuse object with a centrally concentrated luminosity profile, suggesting a relatively smooth morphology. The color appears to transition from a slightly bluer hue in the outer regions to a redder hue in the central core. The shape seems to be somewhat elongated, but not highly so, suggesting a disk-like component viewed at an angle or a mild elliptical shape. There is no obvious evidence of strong spiral arm structure or active merging events. The galaxy may be undergoing a low level of star formation.
