The galaxy presents an elongated, cigar-shaped morphology. The main body appears relatively smooth with a concentrated central region exhibiting a yellowish hue, potentially indicating an older stellar population. Fainter, bluer extensions emanate from either end of the central region, suggesting the presence of younger stars or ongoing star formation activity within a disk-like structure. There appears to be a possible minor disturbance or tidal feature in the region above the galaxy, but this is uncertain. The overall structure does not appear to be involved in a major merger, but does show some evidence of disturbance.
