The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a mostly elliptical morphology, with a high degree of roundness. A slight extension or plume is visible on one side, suggesting a possible tidal feature or interaction. The core of the galaxy shows a yellowish-orange hue, potentially indicating an older stellar population. The outer regions of the galaxy show a faint blue color gradient that may indicate younger stars. The galaxy appears to be relatively isolated with little to no nearby merging partners, though its plume suggests recent interaction.
