The galaxy presents as a somewhat elongated, lenticular-like system. Its morphology is predominantly smooth with a slight hint of a disk component. The color distribution suggests a mix of stellar populations, with a central concentration of older, yellow to orange stars. There appears to be little active star formation occurring within the galaxy, as evidenced by the lack of strong blue colors or distinct HII regions. The overall shape is more cigar shaped, with no indication of spiral arms or a distinct bulge. There is some evidence of minor tidal disturbance that may suggest possible past interactions with a neighbor.
