The galaxy presents a generally smooth and rounded morphology. It appears as a single concentrated object, with a bright, centrally located luminosity. The galaxy seems to be comprised primarily of older stellar populations, and exhibits a spheroidal shape. There is a notable absence of defined spiral arms. The red-shifted nature suggests the galaxy is relatively distant. There are some indications of minor disturbances or potential merger activity, as evidenced by a slight asymmetry and the presence of faint, diffuse light extending outward from the main body, but it is mostly undisturbed. Overall, this is likely a fairly massive, evolved galaxy.
