The galaxy presents a generally smooth morphology, appearing largely elliptical in shape. Its color profile indicates an older stellar population, with a noticeable concentration of light towards the central bulge. There is some suggestion of possible minor disturbances in the galaxy's structure, with faint irregularities in the outer regions. However, it appears to be a relatively settled system without a strong indication of current major merger activity, but perhaps a past event. The overall light distribution suggests a substantial mass, with an older population of stars dominating its composition.
