The galaxy presents as an elongated structure, suggesting an elliptical morphology, or possibly a spiral viewed edge-on. It exhibits a relatively smooth overall appearance, lacking distinct spiral arms or prominent dust lanes. The central region appears brighter and more concentrated, indicative of a bulge. There is a distinct yellowish or reddish hue, concentrated towards the center, possibly signifying an older stellar population. The outer regions show a fainter, bluish tint, potentially indicative of ongoing, though diminished, star formation. There are indications of a possible tidal feature or minor disturbance in the outer halo. There could be ongoing or recent galaxy merger activity.
