The galaxy presents as a relatively smooth, centrally concentrated structure. Its morphology is generally round, showing no apparent strong distortions or tidal features indicative of a recent major merger. A slight extension of the central brightness towards one direction may point to some minor interaction. The central region of the galaxy appears luminous, with a color profile that is generally blue-green. The color becomes redder moving towards the periphery. Given the apparent smoothness of the light distribution, the galaxy is likely an elliptical or lenticular type, with a dominant bulge component and relatively little ongoing star formation.
