The galaxy appears to be a relatively small, disk-shaped system, seen at an oblique angle. The central region exhibits a brighter, more concentrated luminosity profile, suggesting the presence of a galactic bulge. The disk component appears smooth and somewhat diffuse, with a subtle color gradient from the center outwards. There is little evidence of distinct spiral arm structures or prominent star-forming regions within the disk. The galaxy does not show any obvious signs of major tidal disturbances or interactions with other galaxies. The overall morphology appears consistent with a relatively quiescent galaxy with a low star formation rate.