The galaxy presents a discernible disk structure, viewed at an oblique angle relative to its rotational plane. There is evidence of spiral arm morphology within the disk, albeit somewhat flocculent and not sharply defined. The central bulge region appears moderately prominent and exhibits a yellowish hue, possibly indicative of an older stellar population. The disk component displays a bluer color, suggestive of ongoing star formation. There are no signs of strong bar structure. No obvious tidal features or indications of a major ongoing merger are readily apparent, though minor disturbances in the galactic structure cannot be entirely ruled out.
