The galaxy presents as a generally smooth, elliptical structure with a bright, concentrated central bulge. The light distribution appears centrally condensed with a diffuse outer halo. The galaxy appears to be relatively isolated with no obvious signs of major interaction or recent merger activity. There is a slight distortion in the galaxy shape that could potentially be caused by a tidal interaction. The colours seem to indicate an older stellar population, particularly within the core, with a subtle bluer hue in the outer regions indicating perhaps a small amount of more recent star formation. The estimated size of the galaxy is approximately 4 kpc.
