This galaxy presents as an edge-on spiral, exhibiting a high degree of flattening. The central bulge appears prominent, characterized by a yellowish-white hue, suggesting a population of older stars. The disk is visible as a faint, reddish band extending from the central bulge, likely due to the presence of dust lanes and cooler, redder stars. The lack of distinct spiral arm structures and patchy blue regions indicates relatively low star formation activity. No tidal features or signs of recent mergers are apparent. The galaxy's morphology suggests it is an evolved spiral system with a significant spheroidal component.
