The galaxy exhibits an elongated, cigar-shaped morphology. A central bulge region displays a yellowish-orange hue, suggesting an older stellar population. Surrounding this core, fainter, bluish-white regions extend outwards, hinting at the presence of younger stars and potentially ongoing star formation, although at a relatively low rate given the overall color profile. There may be a faint disk structure present, but the image resolution does not allow for a definitive identification of spiral arms or distinct features within the disk. The galaxy appears to be relatively isolated, without signs of major tidal disturbances or ongoing mergers, but there may be minor distortions in its shape, indicating a possible past interaction. The smooth appearance suggests a high degree of radial symmetry, though it may be a disk galaxy viewed at a high inclination angle. The color profile suggests the galaxy has an intermediate mass. 
