The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge which is yellowish-white in color, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes within the observed image. The light appears to gradually fade outwards from the core with the overall shape closely resembling an oblate spheroid. Faint wisps of blue light can be observed at the fringes of the galaxy. This could indicate areas of younger star formation. There are no signs of tidal tails or prominent interactions with other galaxies, implying that it has not recently undergone a major merger event. The general morphology suggests it is a well-formed, relatively undisturbed galaxy.
