The galaxy presents an overall smooth and somewhat elliptical morphology. Its light profile appears to be dominated by an older stellar population, exhibiting a yellowish hue that suggests a relative absence of recent star formation. There is a slight elongation evident, but it largely appears round. The galaxy does not appear to be undergoing any major merging events, though there are some minor indications of possible disturbance in the outer regions, this however is quite subtle. Given the redshift, this galaxy is likely to be a fairly massive system. The absolute magnitudes suggest a bright galaxy. The estimated star formation rate appears to be low, supporting the visual assessment of an older stellar population. The mass estimates indicate it to be a substantial galaxy with an evolved, relatively quiescent nature.
