The galaxy presents as a centrally concentrated object, appearing largely spheroidal. Its light profile seems smooth and relatively featureless, with a gradual falloff in intensity from the core to its outer edges. The dominant color is a pale, somewhat cyan hue, which may indicate a population of older stars or could be influenced by redshift effects at its approximate distance. There is no apparent spiral structure, dust lanes, or other distinct features. A lack of tidal tails or obvious distortions suggests the galaxy is not currently undergoing a major merger event. It is a relatively isolated system, showing no sign of interaction with other galaxies in its immediate vicinity.