The galaxy presents a generally smooth morphology, appearing largely featureless at this resolution. It exhibits a concentrated central bulge, grading into a fainter, more diffuse halo. The overall shape tends towards round, with only a slight deviation from perfect circularity discernible. A faint disk may be present around the bulge, though it is difficult to tell. No signs of tidal tails or major disturbances are apparent, suggesting a quiescent evolutionary state with no recent major mergers. The galaxy exhibits a colour gradient, being more yellow/orange near the core and bluer in the outer regions. This might be due to older stellar populations concentrated in the bulge and younger stars in the more extended regions. The colour differences are slight but present. The relatively small angular size of the galaxy suggests a considerable distance.
