The galaxy presents as a relatively smooth object, exhibiting a centrally concentrated brightness profile. It appears largely elliptical in shape, displaying a high degree of roundness. There is no apparent spiral structure or significant disk component visible in this image. Minor irregularities may be present in the outer regions, suggesting the possibility of tidal interactions or minor disturbances. The object's color is predominantly a slightly bluish-white, indicating the presence of some younger stellar populations, although a significant fraction of older stars likely contribute to the overall luminosity. The galaxy does not appear to be undergoing a major merger, but subtle features hint at potential past or ongoing interactions. There is no central bulge apparent. The rate of star formation is relatively low, possibly due to the consumption of gas reserves or the influence of its environment. The galaxy is of intermediate mass.
