The galaxy exhibits a pronounced disk-like morphology, observed edge-on relative to our line of sight. A central bulge is apparent, displaying a rounded structure with an elliptical profile. The disk shows evidence of internal structure and potential dust lanes, although the image resolution limits detailed characterization. There appears to be limited morphological evidence of ongoing or recent major merger activity. The color suggests a composite stellar population, likely dominated by evolved stars in the bulge, with some evidence of younger, star-forming regions within the disk.
