This galaxy exhibits a relatively smooth morphology, with a dominant, centrally concentrated bulge. The galaxy appears more elongated than circular, tending toward an elliptical shape, but is not distinctly cigar-shaped. There is a subtle suggestion of a disk-like structure. The overall color profile indicates a population of older stars with a yellow-red hue in the central bulge and a more blue-ish tint further along the faint disk. A subtle disturbance in the galaxy's structure is observed. No distinct merger is observed, although there are some signs that there may have been a prior minor interaction with another galaxy. 
