The galaxy presents as a relatively compact object. It appears to exhibit a somewhat elongated morphology, not entirely spherical, with an approximate ratio of 1:2. The primary component of the galaxy shows a bright, concentrated central region which suggests a relatively high density of stars. The galaxy also contains a small, but distinct secondary component that is potentially a satellite galaxy or major star forming region. The overall color profile suggests the presence of both older stellar populations, visible throughout the galaxy, and younger, blue stars concentrated in the more luminous central region.
