The galaxy presents a primarily smooth morphology, with a faint, diffuse halo. The overall shape is elongated, appearing cigar-shaped. A slight suggestion of a disk or spiral structure is noted, but the lack of clear, defined arms indicates a more elliptical or lenticular classification. The color distribution reveals a central region exhibiting a yellowish hue, likely indicating an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of younger, hotter stars. Overall, the galaxy appears to be relatively isolated, showing no obvious signs of a recent major merger, although a minor disturbance cannot be ruled out.
