The galaxy appears to be a relatively smooth, elliptical type, with a concentrated central bulge.  It is somewhat round in shape. The color profile indicates a dominant population of older stars, with a moderate amount of ongoing star formation, which gives the galaxy its light blue appearance. There are no distinct spiral arms or bar structure visible. There is no apparent dust lane obscuring the nucleus. There are no signs of any recent merger activity or tidal disturbances, suggesting a relatively undisturbed evolutionary history.