The galaxy presents a generally smooth morphology, appearing somewhat elongated in shape. There is a bright, concentrated central bulge or core region. The overall color suggests ongoing or recent star formation activity, with the blue-ish color indicative of a population of younger, hotter stars. Faint, diffuse extensions appear around the central region. These extensions are subtle and may be the result of tidal interactions or outflow. There seems to be evidence of a disk, the galaxy is unlikely to be a perfect spheroid. There appears to be some slight disturbance in the form of what looks like minor tidal activity. It does not appear to be undergoing any significant merging events.
