This galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity, transitioning gradually to a fainter halo. There is minimal evidence of spiral arm structures or significant dust lanes, but there is a slight asymmetry in the overall shape, and an irregularity in the edges. The color profile suggests a population of older stars, with a redder hue dominant throughout the galaxy. There are very faint hints of blue regions, but the redness indicates that active star formation is probably slow or has already ceased. There is no distinct nucleus visible at this resolution. The light distribution indicates a relatively smooth stellar distribution, typical of elliptical galaxies.
