This galaxy exhibits a generally smooth morphology with a slight elongation, appearing somewhere between round and elliptical. The central bulge is prominent and displays a concentrated, yellowish-orange hue, suggestive of an older stellar population. Fainter, diffuse, bluish regions extend outwards from the central bulge, indicating the presence of some younger, star-forming regions within the galactic disk. These areas do not exhibit a well-defined spiral structure, but rather appear as irregular patches scattered within the galaxy's outer regions. There is no apparent strong tidal interaction or major merger event visible, though the presence of some subtle asymmetries or minor disturbances within the outer regions cannot be ruled out from this image alone. The overall color profile suggests a galaxy in a transitional phase, moving away from active star formation toward a redder, more quiescent state.
