The galaxy appears as a somewhat elongated, luminous structure with a prominent central bulge. The color profile suggests a higher concentration of older stellar populations, indicated by the yellowish hue of the central region. The outer regions exhibit a fainter, bluish tint, possibly indicating the presence of some younger stars, but these are very subtle. The overall morphology is relatively smooth with no apparent spiral arm structure or signs of major disturbances. Based on these characteristics, the galaxy is likely an elliptical galaxy, or perhaps a lenticular galaxy seen edge-on. There is no evidence of significant ongoing star formation.
