The galaxy presents a generally smooth morphology, with a dominant central bulge. There is some visual evidence of a disk-like structure, though it appears relatively indistinct. The color gradient suggests a higher concentration of older stellar populations. The overall shape approximates a circular form, exhibiting a relatively high degree of central concentration. Some disturbances seem present, though whether caused by tidal interactions or internal processes remains ambiguous. The galaxy is relatively compact, with an estimated effective radius of approximately 7.7 kpc. The galaxy's color indices indicates the galaxy has ongoing star formation. It appears that this galaxy is likely to be an elliptical galaxy with low star formation.
