The galaxy presents a relatively smooth and rounded morphology, exhibiting a dominant central bulge. The light distribution suggests a spheroid-like structure. There appears to be a faint disc component to the galaxy as well, but its morphology is difficult to ascertain with more detail due to image quality. There is a subtle indication of an interaction or disturbance of some kind occurring. Further observation would be needed to confirm this. The galaxy demonstrates a redder color profile, indicative of a stellar population dominated by older stars. Given the observed color, morphology, and possible interacting component, the galaxy is likely an intermediate-mass system with a relatively low star formation rate.
