The galaxy presents an elongated, cigar-shaped morphology. A dominant central bulge exhibits a smooth, yellowish hue, potentially indicative of an older stellar population with lower star formation rates. Surrounding this core, a fainter, somewhat irregular disk-like structure is visible. The disk displays a bluer coloration, suggesting the presence of younger stars and ongoing star formation. There may be signs of minor tidal disturbance or a close interaction, as the disk appears slightly warped or asymmetrical. A small, distinct region of enhanced brightness is visible toward the edge of the disk, possibly a concentrated star-forming region or a smaller galaxy involved in a minor merger. Overall, the galaxy appears to be a transitioning system, potentially evolving from a disk-dominated morphology towards a more spheroid-dominated form.
