The galaxy appears as a roughly circular, centrally concentrated object. The light distribution is relatively smooth with no obvious spiral arms or bar structure. The color profile suggests a dominant population of older stars, indicated by the yellowish hue. There may be a very slight extension or faint halo of material surrounding the main body of the galaxy, but the contrast is low. There is no evidence of ongoing major mergers or significant tidal disturbances. The galaxy seems to be fairly isolated.
