The galaxy presents a concentrated central bulge region with a relatively smooth overall morphology. The luminosity is dominated by the yellow/red wavelengths, hinting at a considerable population of older stars and/or dust obscuration. There are some hints of bluer light emanating from the outer regions which may denote regions of active star formation, but this is marginal. The overall shape is close to round and smooth. There is some evidence of possible minor disturbances, but not enough to suggest a major interaction. The faintness and smoothness of the galaxy suggest an elliptical galaxy that is in the intermediate to later stages of its evolution.
