The galaxy presents as a single, moderately concentrated object, with a fairly symmetrical, elliptical shape. The light profile appears smooth, lacking prominent spiral arm structures or distinct features such as dust lanes. The galaxy exhibits a radial color gradient, transitioning from a yellowish-orange core to slightly bluer outer regions. This suggests the presence of a population of older, redder stars concentrated in the center, with relatively younger, bluer stars towards the periphery. There is no evidence of ongoing major merging activity or significant tidal distortions. The faint, extended halo of diffuse light implies a relatively large spatial extent.
