The galaxy exhibits a relatively smooth morphology, lacking prominent spiral arms or a distinct bar structure. The overall shape appears largely elliptical, although some irregularity is present. A noticeable color gradient exists, with a bluer hue concentrated towards the central region, potentially indicating ongoing star formation. The outer regions appear redder, suggesting an older stellar population. There is some indication of minor gravitational disturbance as the main body seems asymmetrical. No signs of strong tidal tails or major merger events are visually apparent.
