The galaxy appears to be an elliptical morphology, exhibiting a smooth, concentrated light profile. There is a central, bright core that dominates the overall luminosity. The isophotes appear generally elliptical. There may be a slight asymmetry or minor disturbance visible along the edges, but overall there is no strong evidence of ongoing major merger activity. Color gradients exist within the galaxy; the central region appears more yellow, while the outer regions are redder. This color difference suggests a potential variation in stellar populations or dust content between the galactic center and its outer parts. There are no clearly discernible spiral arms or a prominent disk structure.
