The galaxy presents as a somewhat elliptical structure. A bright, concentrated central bulge is apparent, surrounded by a more diffuse disk. The disk appears relatively smooth with subtle color variations suggesting differences in stellar populations or dust distribution. There is a slight indication of the disk being inclined relative to our line of sight. No prominent spiral arm structure is immediately visible. The overall color suggests the galaxy is likely to be a mix of intermediate-age to older stellar populations. Evidence of minor disturbances is not very clear, but not discounted. 
