This galaxy exhibits a primarily smooth morphology, with a highly concentrated central bulge. It presents an overall elliptical appearance, with an approximate diameter of 5 kpc. Evident is a faint, diffuse halo surrounding the bulge. The color profile suggests an older stellar population within the bulge, indicated by the redder hue. There appear to be possible tidal features or disturbances visible, potentially indicative of a minor interaction or past merger event. This is suggested by the irregular shapes of the disturbances and the offset color. The galaxy is also somewhat isolated, with no other major galaxies in close proximity.
