This galaxy appears to be an elliptical galaxy, likely at a considerable distance. It exhibits a generally smooth morphology with no apparent spiral arm structure or significant dust lanes. The galaxy's core is concentrated and luminous, displaying a yellowish-orange hue, suggesting an older stellar population with a lower rate of on-going star formation. The overall shape is highly rounded, lacking any significant elongation. There are no obvious signs of tidal disturbances or interactions with other galaxies. Faint green and red fringing could indicate minimal, but extant, active star formation regions. The galaxy appears relatively isolated within its immediate environment.