The galaxy presents as an edge-on spiral with a prominent bulge. The bulge appears smooth and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. The disk component, viewed nearly edge-on, is elongated and appears relatively thin. There is no evidence of strong dust lanes or significant star formation regions visible in this image, although limited resolution may obscure finer details. The absence of distinct features suggests a relatively quiescent or passive galaxy. The galaxy appears isolated, showing no obvious signs of tidal interactions or merging activity with other nearby galaxies.
