The galaxy presents an elliptical morphology with a smooth, concentrated luminosity profile. It exhibits a yellowish hue in its central region, possibly indicative of an older stellar population. There is evidence of a faint disk. The outer regions appear bluer, which might indicate the presence of younger stars or ongoing star formation. The galaxy does not show any major disturbances or signs of a recent major merger event, but it does appear to be undergoing minor disturbances. The general roundness is in between a circle and a cigar.
