The galaxy presents as a spiral type, with a disk-like morphology oriented approximately face-on. Two distinct spiral arms are visible. The spiral arms exhibit a medium winding, displaying a somewhat flocculent structure with regions of increased luminosity potentially indicating areas of active star formation. The central bulge appears substantial in size, but not excessively dominant compared to the overall disk. The bulge exhibits a smooth, featureless texture and a yellowish-white color, suggesting an older stellar population. The galaxy lacks any obvious strong bar structure across the central region. There are no significant indications of major mergers or strong tidal disturbances in the immediate vicinity of the galaxy. The overall color of the galaxy appears bluish with regions of reddish hues, indicative of a mix of stellar populations.
