The galaxy exhibits a clear disk-like morphology, oriented edge-on from our vantage point. The central bulge appears prominent and elongated. The bulge's light distribution suggests a rounded shape rather than a boxy or non-existent structure. Dust lanes are faintly visible near the central region, obscuring some of the light from the bulge and disk. A region of blue light, possibly indicative of more recent star formation, appears to be located to the left of the main disk, suggesting a possible interaction or merger. Overall, the galaxy demonstrates characteristics of ongoing or recent interactions that could be influencing its structure and star formation activity.
