The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated with a bright, yellowish core that gradually diffuses outwards. The overall shape appears close to round, with minimal elongation. There is no clear evidence of spiral arm structure or a distinct galactic disk. Subtle color gradients suggest the presence of different stellar populations; the core exhibits a greater concentration of older, redder stars, while the outer regions have traces of bluer hues, potentially indicating younger stars, but these features are not prominent. There is a very slight suggestion of minor tidal disturbance, but this is not definitively observable. The galaxy appears relatively isolated with no obvious signs of interaction or recent mergers.
