The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual falloff in surface brightness towards the outer regions. The galaxy exhibits a yellowish-white color, suggestive of an older stellar population. There is very little evidence of prominent spiral arms, dust lanes, or ongoing star formation within the galaxy. The overall round shape indicates a minimal degree of rotational support. No signs of tidal disturbances or interaction with neighboring galaxies are apparent. It is a fairly compact galaxy for its distance.
