The galaxy presents as a somewhat elongated, lenticular structure with a smooth, diffuse light distribution. There is no obvious spiral arm structure or prominent dust lanes visible. The central region appears slightly brighter than the outer regions, but there is no distinct, compact nucleus. The galaxy exhibits a color gradient, appearing bluer towards the edges and redder towards the center. No signs of any major merging events, tidal tails, or significant morphological disturbances. It is relatively isolated in this field, with no obvious nearby interacting galaxies.
