The galaxy presents as a centrally concentrated object with a generally smooth morphology. A distinct, bright nucleus is observed, surrounded by a more diffuse halo or bulge. The light distribution appears relatively even, with no obvious spiral arm structure or strong asymmetries visible in this image. The overall color appears to be tending towards redder wavelengths, and may indicate an older stellar population and a decreased rate of star formation. There may be some weak evidence of a disk structure. There is no evidence of any major merger events.
