This galaxy presents a largely smooth, elliptical morphology. There is an absence of spiral arms or prominent disk structures, lending it an overall spheroidal appearance. The core of the galaxy exhibits a high degree of luminosity, fading into a relatively homogenous halo that appears to have a slightly oblate spheroidal shape. Color gradients indicate a potentially older stellar population, with a yellowish tint overall. There is no evidence of ongoing major merging activity or significant tidal disturbances. It is relatively isolated, lacking obvious interaction with nearby galaxies.
