The galaxy presents as a centrally concentrated system with a smooth, largely featureless morphology. The dominant light is emitted from a spheroidal bulge, exhibiting a yellowish-red hue. The outer regions of the galaxy appear to be enveloped by a faint, diffuse halo displaying a subtle bluish tint. There is no indication of a well-defined disk structure or prominent spiral arms. The galaxy's overall shape is close to circular, showing no obvious signs of significant tidal disturbances or ongoing major mergers. There is, however, a slight asymmetry in the outer halo that may be indicative of minor interactions.
