This galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical with a very high degree of axial symmetry. There is a distinct central bulge region which exhibits a yellow-white color, suggestive of an older stellar population. The outer regions of the galaxy are more diffuse and appear blue, indicating a population of younger, hotter stars and likely some ongoing star formation. There are no obvious signs of spiral arms or a prominent disk structure. The galaxy does not appear to be undergoing any major merging events, with no tidal tails or significant distortions visible. It exhibits an overall red shift indicating it is moving away from our location.
