The galaxy presents an elongated morphology, suggestive of a disk galaxy viewed at a relatively high inclination angle. The central region exhibits a bright, concentrated bulge. The luminosity profile appears smooth and centrally peaked, though there is a degree of asymmetry along the major axis. Color gradients are subtle, with a slightly bluer hue observed in the outermost regions compared to the redder central bulge, suggesting a difference in stellar populations. The disk appears to be disrupted, possibly due to a gravitational interaction or recent merger, with an indication of tidal features or distorted spiral arms. Given the degree of asymmetry, further investigation into the merger history and internal dynamics of this system would be warranted.
