The galaxy presents as a relatively smooth and rounded structure. There is a central, bright core that gradually diffuses outwards. The color profile suggests an older stellar population dominating the galaxy's composition, leaning towards redder hues throughout. No distinct spiral arm structures or significant dust lanes are readily apparent. There might be a hint of a disk-like structure around the center, but it's not very distinct. The overall morphology appears undisturbed, with no obvious signs of major mergers or tidal interactions affecting its shape. The galaxy exhibits a relatively compact form, with a fuzzy edge indicating a gradual decrease in stellar density.
