The galaxy appears to be a relatively smooth, elongated system, exhibiting an overall elliptical shape. A bright, concentrated central bulge dominates the morphology, fading outwards into a less distinct, diffuse disk. The color gradient suggests an aging stellar population concentrated in the bulge, with a shift towards bluer hues in the outer regions, possibly indicating more recent star formation. No prominent spiral arm structures are discernible. There are no obvious signs of a major merger event, although there might be a slight asymmetry to the outer edges. There may be evidence of a minor disturbance based on small visual irregularities. The galaxy is observed at a redshift suggesting a moderate distance. 
