The galaxy presents as a relatively smooth, elliptical-like structure. The core region exhibits a slightly brighter luminosity, transitioning outwards into a more diffuse halo. There is a slight elongation, though it doesn't show a particularly cigar-like shape. There is no obvious spiral arm structure, nor any prominent features indicating active merging. The overall color is a blend of blue and red, with blue light concentrated in the center, suggesting the presence of both young and old stellar populations. There is little evidence of active star formation or dust lanes. There is a subtle asymmetry in the light distribution, which could hint at a minor tidal interaction, but the source is not obvious.
