The galaxy presents as a moderately luminous system, with a resolved structure implying a substantial stellar population. Its morphology suggests a disk galaxy, albeit one observed at an oblique angle such that the disk appears foreshortened and almost elliptical. The primary color appears yellowish/gold, which may be indicative of an older stellar population, but there also seems to be some bluer regions that can be the result of the presence of younger stars and/or star forming regions. The galaxy appears largely undisturbed, with no obvious signs of recent major mergers or tidal interactions. This does not preclude minor interactions or accretion events however. Overall, the object exhibits characteristics consistent with a spiral galaxy undergoing relatively quiescent evolution.
