The galaxy presents as an elongated, cigar-shaped structure with a moderately smooth appearance. The central region exhibits a concentrated luminosity gradient, appearing as a bright, yellowish core, suggesting an older stellar population. Fainter, bluer hues are present at the periphery of the galactic disk, possibly indicating ongoing star formation regions. The overall morphology suggests a disk galaxy viewed at a significant inclination. There is no obvious evidence of major tidal interactions or recent mergers, although subtle asymmetries in the outer regions cannot be entirely ruled out. The general structure indicates it may be a large galaxy.
