The galaxy presents as an edge-on disk galaxy, exhibiting a clear, thin disk profile. The central bulge appears prominent, displaying a smooth, rounded morphology. There is no noticeable dust lane obscuring the central region. The color distribution indicates a concentration of older stellar populations in the bulge, trending toward redder hues, while the disk appears slightly bluer, suggesting the presence of younger, hotter stars and ongoing star formation. There is some indication of a possible tidal feature or minor disturbance, potentially suggesting a past or ongoing interaction with another galaxy, although further spectroscopic analysis would be needed to confirm this hypothesis. It has a considerable mass and a very low amount of star formation occuring within it.
