The galaxy presents as a relatively smooth, elliptical morphology with a concentrated, bright core. The light appears yellowish, indicating a population of older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or strong tidal disturbances, presenting a generally undisturbed structure. Given its red color, it is likely relatively massive, with a significant fraction of its stars past their peak star formation activity. It appears largely spheroidal, with a high degree of central concentration.
