The galaxy appears as a relatively bright, centrally concentrated object. Its light profile suggests a smooth morphology, with no obvious spiral arms or bar structures. The galaxy presents an elliptical shape, leaning towards a more spheroidal form, but not perfectly round. There is little evidence of significant dust lanes or patches. The color is generally consistent across the galaxy, with a slight reddening towards the center. No major ongoing mergers or tidal disturbances are evident, and the galaxy seems relatively undisturbed. Given its color and morphology, it is likely comprised mostly of older stellar populations, and exhibits a relatively low rate of star formation. The galaxy appears to be a relatively massive object, likely residing within a more significant dark matter halo.
