The galaxy presents as a generally smooth, centrally concentrated object, with a slight elongation that suggests it may be classified as an elliptical or lenticular galaxy. A faint blueish hue is evident in the outer regions of the galactic disk. This subtle color variation hints at the presence of a small population of younger, hotter stars in the outer edges of the disk, though older stars still seem to be the dominate population. The galaxy exhibits a slight degree of asymmetry. There is no prominent evidence of active star formation, though the blueish hue hints at some ongoing activity. There is no obvious dust lane or spiral structure within the galaxy's morphology. There is no clear evidence of a major merger event or significant tidal disturbance in its appearance. Overall, the galaxy appears to be a relatively evolved system, potentially in the later stages of its life cycle.
