The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile with no distinct spiral arms or bar structure visible. The light is brightest and most concentrated towards the galactic center, gradually fading outwards. There is a slight elongation to the galaxy's shape. The color gradient indicates a population of older stars dominating the galaxy. There is a lack of blue light, suggesting low levels of ongoing star formation. There is no indication of any major merging events occurring, nor any strong tidal features. There are no significant dust lanes visible. It is possible the galaxy is undergoing, or has ceased, star formation.
