The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated central bulge, which transitions gradually to a diffuse outer halo. The color profile suggests a dominant population of older stars, evidenced by the reddish-orange hue. There is no apparent spiral structure or distinct dust lanes visible. The overall morphology is generally round. No signs of recent major merger events are apparent, although there is a possibility of minor tidal disturbances. Star formation appears to be relatively suppressed throughout the galaxy.
