The galaxy presents as a relatively bright, disk-shaped structure, with an inclination suggestive of an edge-on or nearly edge-on orientation. A distinct central bulge is observed, appearing smooth and concentrated. Evidence suggests a relatively large size. The disk component displays a mottled texture, potentially indicative of spiral arm fragments or dust lane obscuration. A fainter object is seen nearby, and may be interacting with the main galaxy. The color profile appears to display a mixture of older stellar populations and potentially some regions of ongoing or recent star formation. There is also evidence of some tidal disruptions and potential merging activity.
