The observed galaxy presents as a spiral type. The spiral arms are prominent and well-defined, exhibiting a relatively open structure. They appear somewhat flocculent with indications of active star formation regions along their lengths, indicated by a bluish tint. The central bulge is relatively small but distinct, displaying a yellowish hue suggestive of an older stellar population. The galaxy disk is inclined to our line of sight, giving it an elongated shape. There is no obvious presence of a strong bar feature within the galaxy. Some minor disturbances may be present in the outer regions of the spiral arms. Overall, the galaxy is likely a spiral galaxy exhibiting moderate ongoing star formation.
