The galaxy presents as a relatively smooth, elliptical-like object. The central bulge is prominent and exhibits a concentrated, yellowish hue, suggesting a population of older stars. A flattened disk component is suggested as there appears to be a plane visible, however this is subtle. There does not appear to be any spiral arm structure or significant dust lanes visible within the disk. The galaxy displays a fairly high degree of symmetry. No major signs of tidal disturbances or ongoing mergers are readily apparent. There may be some faint, minor irregularities in the outer regions of the disk, but these are not well-defined. Overall, the galaxy appears to be a fairly undisturbed, evolved system.
