The galaxy presents as an edge-on disk galaxy. A prominent bulge is observed, appearing rounded in shape, dominating the visual morphology. The disk component exhibits a relatively smooth texture, showing no clear signs of distinct spiral arm structures or significant dust lanes. The overall color profile suggests a stellar population that is relatively old, as indicated by the yellowish hue. The lack of bright blue regions implies a low rate of ongoing star formation. The galaxy does not appear to be undergoing any significant merging activity, with no major disturbances visible in its structure.
