The galaxy appears as a centrally concentrated, somewhat elliptical object. It exhibits a smooth morphology with a dominant, round central bulge characterized by a redder hue, likely indicative of an older stellar population. Fainter, bluer light extends outwards from the core, particularly towards the lower-left in the image. There may be a hint of a disk structure, but the dominant impression is that of a spheroid galaxy. There is no clear evidence of spiral arms or strong tidal disturbances, suggesting that the galaxy is relatively undisturbed dynamically. There might be some slight asymmetry or minor disturbance, though the image quality prevents a definite assessment.
