The galaxy presents a generally smooth and elliptical morphology. There appears to be a central, highly luminous bulge, exhibiting a yellowish-orange hue. The light from the central bulge dominates the visual appearance of the galaxy. Extending outward from the core, there is evidence of a faint disk or envelope. This outer region has a bluer color profile compared to the core, suggesting the presence of a younger stellar population and ongoing star formation. There are no obvious signs of strong tidal disturbances or major mergers. The overall structure indicates a galaxy that may be in the process of transitioning from a star-forming spiral to a more quiescent elliptical type, but continues to exhibit low levels of star formation. The shape is generally elliptical with a slight flattening.
