The galaxy presents as a relatively smooth, elliptical or lenticular morphology. Its overall shape is somewhat elongated, though it exhibits significant central concentration of light. The color profile suggests a population of older stars, with a redder hue dominating the central region. There's a slight green tinge, possibly hinting at the presence of some ongoing, albeit limited, star formation activity within the galaxy. No prominent spiral arms or dust lanes are discernible. There is no clear indication of strong tidal interactions or mergers, though a subtle asymmetry cannot be entirely ruled out. The galaxy appears to be relatively isolated in its environment.
