The galaxy exhibits an overall elliptical morphology, with a dominant, smooth central bulge. The color profile suggests a primarily older stellar population, with a redder hue concentrated in the central region. There appears to be some bluer emission, potentially indicating more recent star formation activity, primarily towards the lower portions of the galaxy. Evident is what looks like a possible disturbance or a tidal tail. The galaxy demonstrates relatively little rotational symmetry, as it does not exhibit significant disk-like features or spiral arms. It appears to be relatively undisturbed by any major ongoing mergers, and may be a transitional object slowly quenching and settling into a red and dead phase.
