The galaxy appears as a moderately bright, slightly elongated spheroid. It exhibits a diffuse halo with no readily apparent spiral arm structures or significant dust lanes. The central bulge is not prominently defined, suggesting a relatively even distribution of light intensity across the galactic body. The light emitted from the object suggests that the galaxy has intermediate redshift, with the more red portions of the spectrum being more visible to us. There is also an absence of intense, localized star-forming regions, based on the lack of intensely blue spots. A minor disturbance may be affecting its shape.
