This galaxy exhibits a generally smooth morphology. It appears slightly elongated in shape, with a dominant, relatively bright central bulge that transitions smoothly into the outer regions. The color profile suggests an older stellar population, particularly in the central bulge, which displays a yellowish hue. Moving outwards, the surrounding disc or halo shows bluer tones, which may indicate ongoing or recent star formation activity, although this is not particularly pronounced. There is no clear evidence of spiral arm structure, significant dust lanes, or any major disturbances indicative of a recent merger event, although some minor asymmetry is visible. The overall appearance is consistent with an elliptical galaxy or a lenticular galaxy seen at a considerable distance.
