The galaxy presents as a face-on spiral, exhibiting a well-defined disk structure. Faint spiral arms emanate from the central bulge, appearing tightly wound. The bulge is small relative to the disk. No strong bar feature is apparent. The spiral arms are numerous and not clearly defined. There is no evidence of any major merging or tidal disturbances, but the spiral structure is slightly irregular, possibly indicating a minor interaction. The disk shows a relatively smooth luminosity profile, suggesting it could be dominated by an older stellar population. 
