The galaxy presents as a single, dominant light source with a smooth, elliptical morphology. A strong central bulge is apparent, exhibiting a concentrated, yellowish hue. The overall distribution of light suggests a high degree of radial symmetry. There appears to be little in the way of discernible spiral arm structure or dust lanes. The color suggests an older stellar population with a relatively low ongoing star formation rate. There is no evidence of tidal tails or other significant distortions, suggesting no recent major merger events. The outer regions of the galaxy fade gradually into the background, lacking a sharp boundary.
