The galaxy presents a centrally concentrated morphology, with a significant fraction of its light emanating from a bright, yellowish core. This central region appears relatively smooth and featureless, suggesting an older stellar population. The overall shape is somewhat elliptical, though not perfectly so; it appears slightly disturbed. Fainter, more diffuse material surrounds the core, extending outwards in a somewhat irregular fashion, most notably with a plume-like feature extending from the core. This plume appears bluer in color than the core, potentially indicating more recent star formation. There may be minor disturbances or tidal features present, suggesting a possible interaction or past merger event. The galaxy exhibits a moderate redshift.
