The galaxy exhibits an overall elliptical morphology, appearing elongated with a high degree of oblateness. The central bulge is a prominent, concentrated region of light, appearing a yellowish hue. This suggests a population of older stars. The outer regions of the galaxy display a fainter, bluer color, which may indicate more recent star formation. There is no evidence of a distinct spiral arm structure or a prominent disk component. The galaxy shows minimal signs of tidal disturbances or mergers, appearing relatively undisturbed in its overall structure. Based on the color distribution, it seems that star formation may be suppressed compared to spiral galaxies, with a possible concentration in the outer regions. Overall, the galaxy appears to be an early-type galaxy with minimal active star formation.
