The galaxy presents as a relatively smooth, elliptical object. The core is a bright, concentrated region displaying a yellow hue, suggesting an older stellar population. The light profile gradually diminishes outwards from the core, transitioning to a fainter, reddish halo. There is a very slight suggestion of a disk-like structure or feature. There is no evidence of a recent or ongoing major merger, although the galaxy is slightly elongated in shape, possibly cigar-shaped. There may be a minor gravitational disturbance in the form of a tidal tail or stellar stream.
