The galaxy presents a primarily smooth morphology, appearing as an elongated, cigar-shaped structure. There is a subtle color gradient across the galaxy's body, transitioning from a brighter, more yellowish core to slightly bluer and fainter extremities.  The central region exhibits a concentrated luminosity, potentially indicating a dense stellar population or an active galactic nucleus. While the overall structure is smooth, there is a hint of possible disk-like component. There are no clear signs of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure. Overall, the galaxy appears as a relatively undisturbed system with moderate star formation activity.
