The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a bright, concentrated luminosity, which fades gradually towards the outer regions. It is characterized by a yellow-reddish hue, indicating an older stellar population and reduced levels of ongoing star formation. There is a slight elongation, although the object appears largely spheroidal. No prominent spiral arm structures or dust lanes are discernible in this image. Subtle irregularities in the outer halo suggests a possibility of minor gravitational interactions, though the overall morphology suggests no major recent mergers.
