The galaxy presents as a spiral type, exhibiting a disk-like structure with discernible spiral arms. Two primary arms are visually dominant, curving from the central bulge outwards. The winding of the spiral arms appears to be of medium tightness. 

The central bulge is moderately prominent, displaying a yellowish hue suggestive of an older stellar population. The disk exhibits a bluer color overall, potentially indicating ongoing star formation within the spiral arms. There is a faint suggestion of a bar-like structure spanning across the central region. 

Evidence of tidal disturbances is subtly apparent. The galaxy appears to be isolated with no large objects directly nearby; the tidal disturbances are not the result of any major mergers.
