The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Its overall structure is characterized by a relatively bright central bulge, appearing yellowish-white, surrounded by a flattened disk. Two prominent spiral arms emanate from the central region, exhibiting a relatively tightly wound structure. The arms display regions of bluer light, suggestive of ongoing star formation. The bulge-to-disk ratio appears moderate, with the disk significantly larger than the bulge. There is no indication of a strong bar structure in this image, though some distortion may be possible. The overall color gradient suggests an older stellar population in the central bulge. The image suggests a classification of a spiral galaxy with a somewhat prominent bulge and active star formation within the spiral arms, with no strong evidence of a major merger or strong interactions.
