The galaxy presents a somewhat disturbed morphology. It displays a prominent central bulge region with a reddish hue, possibly indicative of an older stellar population or dust obscuration. Extending from this central region are diffuse, fainter structures suggestive of a disk component, although the disk appears to be somewhat irregular. There are some regions of relatively high brightness extending out from the disk that point to the presence of regions of star formation within the disk. The overall appearance suggests a possible interaction or recent merger event. The faintness of the disk and the apparent irregularity suggest moderate-to-low star formation. The galaxy is roughly elliptical in overall shape, with a slight elongation.
