The galaxy presents as a disk galaxy, oriented nearly edge-on with respect to our line of sight. A prominent central bulge is visible, exhibiting a yellowish-white hue, suggesting a population of older stars. The disk appears relatively smooth, showing a faint, diffuse blueish color. It is likely a spiral galaxy, but the extreme edge-on orientation obscures any clear spiral arm structure. The overall color profile suggests a mature galaxy with a low star formation rate. No signs of a major merger event are evident, though slight irregularities in the disk structure could suggest minor disturbances. The galaxy's size, while difficult to precisely assess due to its orientation, appears moderate.
