The galaxy presents a generally smooth morphology, appearing elliptical or lenticular in shape. The central bulge exhibits a yellowish hue, indicative of an older stellar population. Fainter, bluer light surrounds the central region, perhaps suggesting a low level of ongoing star formation within a disk component. Overall the galaxy is very compact, and the disk appears fairly small relative to the size of the bulge. There are no readily apparent signs of spiral arms or significant dust lanes. Faint irregularities exist in the outer envelope of the galaxy, which could be indicative of minor tidal interactions or past merger events. 
