The galaxy presents as a spiral type, viewed at a significant inclination. Two prominent spiral arms are evident, though tightly wound and somewhat indistinct. A central bulge is visible, appearing moderately sized relative to the overall galactic disk, exhibiting a yellowish hue suggestive of an older stellar population. No obvious bar structure is apparent, but there may be a faint central concentration that requires further investigation. The disk shows a mix of bluer and yellower regions, possibly indicative of ongoing star formation in some areas, with more quiescent regions elsewhere. There is no immediately discernible indication of major tidal distortions or recent merger activity, suggesting a relatively undisturbed evolution. The overall morphology is generally smooth.
