The galaxy presents as a luminous, elliptical or lenticular structure. Its overall form is smooth with a high degree of central concentration, suggesting an older stellar population. The color profile indicates a relatively red hue across the galaxy, which would also suggest a population of older stars. The galaxy appears to be largely undisturbed with no readily apparent signs of ongoing mergers or significant tidal interactions. The general shape appears to be somewhere between round and cigar-shaped.
