The galaxy presents as a somewhat elongated, disk-like structure oriented at a considerable angle to our line of sight. The central region appears bright and concentrated, displaying a yellowish hue suggesting an older stellar population. Moving outward from the core, the disk exhibits a more diffuse structure, with faint extensions in either direction. There's a hint of blue in the extensions, possibly indicative of some star formation. The overall shape is relatively smooth, though subtle irregularities may indicate some past interactions or disturbances. The galaxy's color profile suggests a mix of stellar populations, with an older bulge and potentially younger stars within the disk.
