The galaxy presents as a spiral galaxy, seen at an approximate redshift of z = 0.083320. It exhibits a prominent disk structure with well-defined spiral arms. The spiral arms appear tightly wound around a central bulge region.

The central bulge has a yellowish hue, indicative of an older stellar population. The spiral arms display a bluer color, suggesting ongoing star formation activity. Evidence of star formation is noted in the arms, potentially indicating HII regions or young star clusters.

The galaxy's disk is oriented approximately face-on to our line of sight. There is no apparent dust lane or significant obscuration within the galaxy. There is no clear sign of a strong bar structure bisecting the central bulge. It does not appear to be interacting with another galaxy, nor does it seem to have undergone a recent major merger event as its symmetry is still largely intact.