The galaxy presents as a well-defined, disk-shaped structure viewed nearly edge-on. The central bulge appears prominent, exhibiting a yellowish hue. The disk itself displays a bluer color, suggesting ongoing star formation. No spiral arm structures are clearly visible, likely due to the near edge-on orientation. There is no apparent interaction with neighboring galaxies, as it seems to be relatively isolated. The absence of significant dust lanes is notable, although some obscuration may be present along the equatorial plane. The galaxy appears generally smooth, showing some evidence of a bulge that is not distinctly boxy.
