The galaxy presents an elongated morphology, indicative of a disk galaxy viewed nearly edge-on. A central bulge is visible, characterized by a concentration of light exhibiting a warmer, orange-ish hue, likely indicative of an older stellar population. The disk component extending from the central bulge appears relatively smooth and diffuse. Overall, the disk exhibits a slightly asymmetric structure, possibly due to internal dynamics or interactions. The observed color distribution suggests a moderate level of star formation.
