The galaxy presents as a moderately luminous object with an overall elliptical morphology. A concentrated central bulge is apparent, exhibiting a yellowish hue, suggesting an older stellar population and reduced star formation within the nuclear region. The outer regions display a more diffuse, disk-like structure. Patches of bluer light are visible in the outer disk, indicating regions of ongoing star formation, albeit at a relatively modest rate. There appears to be only a minor disturbance to the main structure of the galaxy. No strong tidal features or signs of recent major merger activity are immediately obvious from the image. The galaxy shows some defined disk features, though it is difficult to confidently determine the presence of spiral arms.
