The galaxy presents a generally elliptical morphology. There is a notable central bulge which seems to be surrounded by a faint ring. The galaxy displays a relatively smooth texture, lacking prominent spiral arms or distinct knots of star formation in the region. The color profile appears to be predominantly green, suggesting a composition of older stars or a significant dust component affecting the wavelengths of light seen here. There is some indication of a central concentration of light, but there are not any obvious disturbances suggesting an ongoing or recent merger event. The outskirts of the galaxy fade gradually into the background sky, indicating a smooth distribution of stellar density.
