This galaxy appears to be a relatively small, low-mass system. Its morphology is elliptical in shape. There is a relatively smooth central bulge with the light being most concentrated at the core. The outer regions of the galaxy are fainter, indicating a decreasing stellar density with increasing radius. There is little indication of spiral arms or other distinct features, suggesting this is either a lenticular or elliptical galaxy, without significant ongoing star formation. It is of a relatively low redshift, indicating it is relatively close to our own galaxy. Its blue coloration may indicate some presence of younger stars, even if a large portion of the population is relatively old. There is likely no on-going merging event with another galaxy or significant disturbances to the system's morphology.