The galaxy presents a primarily smooth and elliptical morphology, exhibiting a concentrated central bulge that radiates with a yellowish hue. This suggests a significant population of older stars. A faint, elongated structure extends from one side of the galaxy, possibly indicative of a tidal tail or a disturbed disk. The galaxy exhibits a slight asymmetry and a faint blueish tinge at the furthest point of its extension. It is a fairly massive galaxy. There is little evidence of current, intense star formation within the central region, as indicated by the lack of bright blue regions typically associated with young, hot stars.