The galaxy exhibits a somewhat elliptical morphology. A bright, concentrated central bulge dominates the visual structure. The bulge appears to transition smoothly into a more diffuse disk, although the disk component is faint and indistinct. There is no indication of a well-defined spiral arm structure, or bar. The color profile suggests a relatively quiescent galaxy, with the overall hue appearing to be a slightly yellowish white. This is consistent with an older stellar population in the bulge and a reduced rate of on-going star formation throughout the galaxy as a whole. Minor tidal disturbances do not appear to be disrupting the galaxy.
