The galaxy presents as a relatively smooth, elliptical object. Its light profile is centrally concentrated, with a bright core that gradually fades into the surrounding halo. The galaxy appears largely featureless, with no prominent spiral arms or dust lanes visible in this image. The overall shape is close to round, exhibiting only a slight elongation. There is no indication of any major mergers or significant tidal disturbances affecting its morphology, although a minor perturbation cannot be ruled out. The observed colors suggest a predominantly older stellar population. We can infer a low star formation rate. The size of the galaxy appears relatively modest, possibly indicating a dwarf or intermediate-mass system.
