The galaxy presents as a somewhat elongated elliptical morphology. Its color appears to be predominantly yellowish-orange, concentrated towards the center, suggesting an older stellar population. The galaxy has a smooth appearance with a relatively high central concentration of light. There is a slight asymmetry in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. Indications show a low amount of star formation activity. There are some minor disturbances on the edges which may be the results of a past or ongoing minor merging event. 
