The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be an elliptical galaxy, exhibiting a diffuse, somewhat round morphology. The color profile suggests a dominant older stellar population, indicated by the yellow-orange hue in the central region. There is a subtle color gradient, shifting towards slightly bluer tones in the outer regions, which could indicate the presence of some younger stars, though the overall star formation rate is likely low. No prominent spiral arms or significant dust lanes are discernible, and the galaxy appears undisturbed, with no major signs of tidal interactions or ongoing mergers. The galaxy's estimated physical size is around 9 kpc, suggesting it is a dwarf galaxy. There may be a supermassive black hole, given its mass.
