The galaxy appears to be largely smooth in morphology. It exhibits a concentrated central bulge, which graduates outwards into a less defined and dimmer halo. The light profile suggests a centrally dominant structure. There is a possible indication of a disk feature, although the blurring in this image makes any definite observation difficult. If there is a disk, it is likely oriented close to face-on. Any spiral arms are not resolved. Overall, it seems to be an unbarred smooth galaxy with no major disturbances from any interactions, perhaps a spiral or lenticular system. There is the potential of minor disturbances in the light profile.
