The galaxy presents a generally smooth morphology, with an elliptical appearance. The central bulge exhibits a distinct yellowish hue, suggesting an older stellar population. Moving outward from the core, there is a subtle gradient towards bluer tones, potentially indicating regions of more recent star formation, albeit at a low rate. The galaxy exhibits only a slight degree of disturbance in its overall structure. Based on its appearance, this galaxy is likely a relatively massive system. The shape is more in-between elliptical and disc.
