The galaxy displays a spiral morphology, characterized by a prominent disk structure. The disk is observed at an oblique angle, presenting a somewhat edge-on view. Two tightly wound spiral arms emanate from a central bulge, exhibiting a degree of asymmetry in their structure. The bulge appears to be of moderate size relative to the overall galaxy. The color distribution suggests active star formation regions within the spiral arms, indicated by a bluer hue, contrasting with the yellower bulge region, which might indicate an older stellar population. The overall luminosity appears moderate. There is evidence of some tidal disruption or a minor merger, potentially perturbing the galactic disk, suggesting some interaction.
