The galaxy presents as a somewhat elongated structure, appearing nearly edge-on from our vantage point. The central bulge exhibits a concentrated, bright yellow-orange hue, indicative of an older stellar population. A fainter, bluer disk extends outward from the bulge, suggesting the presence of ongoing star formation within this region. There appears to be a possible tidal tail or dwarf galaxy in the bottom right with similar yellowish hue. Overall, the galaxy demonstrates a complex morphology. The galaxy's apparent moderate luminosity suggests a significant stellar mass.
