The galaxy presents as a relatively compact object with a smooth, elliptical morphology. There is a slight elongation, however the overall shape is more akin to an oblate spheroid. The central region appears brighter than the surrounding areas. The light distribution suggests a relatively old stellar population. There is little evidence of spiral arms, dust lanes, or active star formation regions. There are no obvious signs of interaction with neighboring galaxies. Overall, the galaxy is likely to be an elliptical galaxy with little active star formation.