The galaxy presents as an elliptical or lenticular morphology, appearing largely featureless and smooth in texture. The core exhibits a bright, concentrated luminosity, suggestive of a high stellar density in the galactic nucleus. There is an absence of prominent spiral arms or dust lanes. The light profile appears to fade gradually from the center outwards, with a slight elongation indicating a deviation from perfect circularity. Faint blue tinges are present towards the outskirts, which may indicate some level of ongoing star formation. There is no clear evidence of any major merger events or significant tidal disturbances in its immediate vicinity. Overall, the galaxy appears to be relatively evolved.
