The galaxy presents as a spiral type, exhibiting a moderately inclined disk. A central bulge is visible, presenting a yellowish-white hue, suggesting an older stellar population. Two well-defined spiral arms emanate from the central bulge, tracing a distinct pattern. The arms display a somewhat flocculent structure with varying intensity. Some degree of symmetry in the arm structure can be appreciated. The disk itself presents a mottled appearance indicative of star forming regions interspersed with areas of dust obscuration. The galaxy does not appear to be undergoing any major merging events.
