The galaxy presents as a moderately inclined disk galaxy with a smooth, centrally concentrated bulge. There is faint blueness observed in the disk suggesting some level of recent or ongoing star formation. The disk appears relatively featureless, with a smooth light distribution and no obvious spiral arm structure is apparent. There is no evidence of a major merger, although some minor tidal disturbance cannot be ruled out given the image resolution. The overall color profile suggests the galaxy consists predominately of older stellar populations but it's still forming a very low amount of stars. The galaxy exhibits an approximately round morphology, indicating that it is not particularly elongated.
