The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge appears relatively smooth and spheroidal. The disk is clearly visible, extending outwards from the bulge, and has a high degree of inclination relative to our line of sight. There is no obvious evidence of a strong bar structure. Faint, elongated dust lanes are potentially present within the disk, although the resolution is not sufficient to definitively confirm their morphology. There are no obvious signs of major mergers or tidal disturbances. Based on its red color, the galaxy likely has a relatively low star formation rate.
