The galaxy presents as a fairly smooth, disk-like structure, though the disk component is only faintly visible. The galaxy exhibits a high degree of central concentration of light, appearing largely spheroidal. The color is generally reddish, with some evidence of a faint disk that has a weak blueish hue. The lack of defined spiral arms or dust lanes suggests a relatively evolved system. It does not obviously display signs of ongoing major mergers, although the light asymmetry could be a sign of minor disturbances. The galaxy's apparent round shape may indicate that we are viewing it close to face-on. Overall, the galaxy appears to be an intermediate-redshift galaxy that is likely of substantial mass and a slow rate of star formation.
