The galaxy presents as a moderately bright, elongated structure, likely a disk galaxy viewed at an oblique angle. The central region exhibits a higher concentration of light, suggesting a prominent bulge or core. This core appears to be slightly offset from the geometric center of the disk. The disk itself shows hints of asymmetry, potentially indicating past or ongoing interactions. The color profile shows a blueish hue, especially in the outer regions, suggesting active star formation. A subtle, diffuse halo surrounds the main body of the galaxy, with some features hinting to minor interactions.
