The galaxy presents a generally smooth and rounded appearance, suggestive of an elliptical morphology. It exhibits a concentrated central region that gradually diffuses outwards. There may be a slight elongation present, though the overall shape is predominantly circular. Color gradients across the galaxy are subtle but present; the central region appears yellower, transitioning to a redder hue in the outer regions. This color gradient might indicate a difference in stellar populations, with older, redder stars dominating the outer regions. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing any major merger events or exhibiting significant tidal distortions. The galaxy's relatively featureless structure suggests that it is a relatively evolved system with a history of quiescent star formation.