The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively spheroidal in shape, although with some elongation. The galaxy displays a color gradient, with a brighter, more yellow core that likely signifies an older stellar population. Fainter, slightly bluer light extends outward from the core, suggesting the presence of some younger stars, or perhaps a faint disk structure, although not particularly pronounced. There is no clear evidence of spiral arms or major disturbances to the galaxy’s structure; it seems mostly undisturbed. Overall, the galaxy has a low rate of star formation. The mass is estimated to be around 10^10 to 10^11 solar masses, which suggests this galaxy is a dwarf galaxy.
