This galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical morphology, though it's orientation is close to edge-on. The galaxy exhibits a central concentration of light that appears to be more red in color, possibly indicating an older stellar population dominating the core. Moving outward from the core, the galaxy appears to have a bluer halo, which could be indicative of ongoing, albeit low, star formation. There is no apparent spiral arm structure or significant dust lane visible. The overall structure indicates a system that is not currently undergoing any major interactions, such as a merger, however, there is a hint of a possible minor disturbance in the outer halo.