The galaxy presents an overall smooth appearance with a centrally concentrated bulge. The shape of the galaxy appears somewhere between round and elongated. There is evidence of a slight disturbance within the galaxy, but no indication of a major merger or significant tidal features. There is subtle color variation, with the central region appearing bluish-white, fading into a more yellow-red hue as it extends outwards. Based on these observations, the galaxy could be classified as an early-type spiral or a lenticular galaxy. The blue-ish center might indicate a low level of star formation activity in the nuclear region.
