The galaxy appears as a moderately luminous, relatively smooth elliptical or lenticular system, with a slightly elongated shape. It exhibits a concentrated central bulge that fades gradually into the outer regions, with no distinct spiral arm structure visible. The galaxy's color is mostly a uniform yellowish-white, indicative of an older stellar population. Evidence suggests a past or ongoing interaction or merger, potentially reflected in the disturbed morphology. The galaxy is of a substantial mass and has low star formation. The object is relatively compact, with a clearly defined core.
