The galaxy presents as a single, smooth structure with a centrally concentrated luminosity profile. It appears largely elliptical in shape, exhibiting a high degree of roundness. The galaxy's color suggests an evolved stellar population, with a yellow-orange hue indicative of older stars. There is a possible minor interaction with a small adjacent galaxy, but that is not fully determinable. There are no obvious dust lanes or spiral arm structures visible. It may be undergoing a minor merger event, but this is not conclusive based on the available data.
