The galaxy presents a generally smooth morphology, with a dominant central bulge. It exhibits a slightly elliptical shape, appearing more rounded than elongated. The color profile suggests a higher concentration of older stellar populations, indicative of a passively evolving system. There is minimal evidence of ongoing star formation within the visible light spectrum, implying a relatively low star formation rate for a galaxy of this mass. Slight color variations may indicate minor internal structure or localized differences in stellar populations, but these are subtle. There do not appear to be any major disturbances or merging events drastically affecting the galaxy's overall structure, although some slight asymmetry cannot be completely ruled out.
