The galaxy presents as a largely smooth, elliptical or spheroidal structure. It exhibits a concentrated, bright core, surrounded by a more diffuse halo or envelope. The color profile suggests an older stellar population, dominated by redder and yellow wavelengths. There is a secondary object in close proximity to the galaxy that may be interacting with the galaxy, or simply another galaxy in the distance. There is little to no evidence of spiral arms or prominent dust lanes. Overall, the galaxy appears to be a relatively evolved system, with a high degree of symmetry.
