The galaxy appears as an elongated, cigar-shaped structure, suggesting it may be an elliptical galaxy. The central region exhibits a bright, diffuse glow, possibly indicating a high concentration of stars. The color gradient transitions from a yellowish-white core to a bluer, fainter outer disk. The galaxy appears relatively smooth, showing little evidence of spiral arms or distinct features typically associated with disk galaxies, though some slight disturbances are present. Overall, the morphology suggests a system dominated by older stellar populations with minimal active star formation.
