The galaxy presents a lenticular morphology, appearing as a flattened disk viewed edge-on. A prominent central bulge is observed, exhibiting a bright, concentrated luminosity profile, possibly indicating an older stellar population. Extending outwards from the bulge is a disk component, appearing relatively smooth with subtle variations in color, suggesting a lack of significant recent star formation. Faint tidal features or distortions are noted which are not obviously indicative of a major merger event. An overall slight blue tint is visible surrounding the disk which may be from smaller star forming areas or artifacts. The aspect ratio is notably elongated, lending further support to its classification as an edge-on disk galaxy.
