This galaxy presents as a disk galaxy, seen nearly edge-on. There is a prominent central bulge that appears yellowish in color, suggesting an older stellar population. The disk itself is also visible, although its structure is not clearly resolved, appearing relatively smooth with some indication of dust lanes. The apparent lack of bright blue regions indicates a low rate of recent star formation. There is no obvious evidence of a major merger or tidal disturbances. Overall, it appears to be a relatively massive galaxy with low specific star formation rate.
