The galaxy presents as a flattened elliptical form, elongated along its major axis. There is a brighter, more concentrated central bulge which appears yellowish, indicating an older stellar population. Diffuse light extends outwards from this central region, fading into the surrounding background. The outer regions of the galaxy lack distinct spiral arm structures. The galaxy appears relatively smooth, with only subtle variations in luminosity across its surface, and appears to be roughly 4.6 kpc in radius. The colour gradients suggest a possible gradient in stellar population density, with older, redder stars concentrated towards the galactic centre. The galaxy appears to be in a relatively isolated location with no immediate signs of tidal disturbances or interaction with other galaxies.
