The galaxy presents as a generally smooth, round object with a concentrated central bulge.  A faint disk component is suspected, showing very subtle structural irregularities, but is not clearly resolved. Color gradients are present, with the central region exhibiting a yellowish hue, transitioning to a bluer tone in the outer regions.  There is no strong evidence of ongoing major mergers, although minor tidal disturbances may be present upon further investigation. The galaxy is dominated by a central bulge with weak disk features. The general appearance is consistent with an early-type spiral or a lenticular galaxy.
