The galaxy presents an overall elliptical morphology, although some disk-like features are weakly suggested. The light distribution appears somewhat smooth, without prominent spiral arms or distinct clumps of star formation. There is a subtle elongation observed, hinting at a cigar-shaped structure. The central region shows a slight concentration of light, possibly indicating the presence of a bulge, however, the image resolution limits further analysis of the galactic nucleus. There is some suggestion of a faint, diffuse halo surrounding the main body of the galaxy. Overall, the galaxy exhibits a quiescent appearance, suggestive of a relatively low star formation rate. There is no clear indication of any major ongoing merger activity, though minor disturbances in the morphology cannot be ruled out. The galaxy exhibits a redder color in the central regions and a bluer tinge near the faint disk, a common sign of star-formation occuring in the disk.
