The galaxy presents as a spiral type with a clearly discernible disk structure. While not perfectly edge-on, the viewing angle is oblique, offering some face-on perspective. A prominent central bulge is observed, appearing relatively bright and concentrated, but not overwhelmingly dominant. Spiral arms are evident, exhibiting a somewhat patchy or flocculent morphology. The galaxy's overall color profile suggests a mix of stellar populations, with the central bulge appearing yellower, potentially indicating older stars, while the disk exhibits bluer hues, suggestive of ongoing star formation. No strong bar feature is immediately apparent. The galaxy does not appear to be undergoing any major merger events, though some minor asymmetries or irregularities could indicate minor interactions or disturbances.
