The galaxy presents as a somewhat elliptical structure, but not perfectly spherical. It is centrally concentrated with a smooth light distribution, hinting at an older stellar population. There is a slight elongation or cigar shape that is hard to confirm, but it gives the galaxy an oval shape that's more in-between elliptical and spherical. The core is very bright. There is the possibility of disturbance, with the core pulling on the rest of the structure. The galaxy appears to be experiencing a minor disturbance. It exhibits a color gradient, with a redder hue concentrated towards the center and a slightly bluer tinge in the outer regions. This suggests potential variations in stellar populations, metallicities or dust content throughout the galaxy. There is no evidence of a spiral structure.
