The galaxy presents as a somewhat elongated structure, possibly a spiral galaxy viewed at an oblique angle. The central region exhibits a concentrated luminosity, appearing yellowish-orange in color, indicative of an older stellar population. Fainter, bluer regions are observed extending from the central bulge, suggesting areas of ongoing star formation. There is a slight lopsidedness in the overall structure. Faint, diffuse emission surrounds the central region, possibly representing a halo or extended disk. The galaxy appears to be relatively isolated with no obvious signs of interaction with other galaxies.
