This galaxy appears to be relatively compact, exhibiting a centrally concentrated morphology. The core region is very bright, with the color profile indicating possible active galactic nucleus contribution, or a region of intense star formation.  Surrounding the bright central area, there is a more diffuse, fainter halo of light.  The overall shape of the galaxy is roughly elliptical, though it may be exhibiting some signs of disturbance or tidal features in its outer regions. There may be indications of possible minor interactions or a recent minor merger event. It does not appear to be a spiral galaxy, nor does it appear to have any noticeable disk structures. The majority of the light is within a radius of approximately 4 arcseconds.
