The galaxy presents as an elongated structure, appearing cigar-shaped. Its light profile indicates a smooth overall morphology, although there is some evidence of a disk-like component. The color gradient suggests a central bulge with older stellar populations, exhibiting a reddish-yellow hue, that fades to a bluer tint along the extended edges, hinting at potential star formation activity within these regions. No significant interactions or major disturbances from nearby galaxies are obvious, though a minor interaction cannot be ruled out.
