The galaxy presents an overall elliptical morphology, with a smooth, diffuse light distribution. There is a high degree of central concentration, with the luminosity decreasing steadily from the core outwards. The galaxy exhibits a moderate redshift, suggesting it is relatively distant. The color profile indicates a predominantly older stellar population, as evidenced by the redder hues. There are no prominent spiral arms or significant dust lanes visible. There might be a very slight asymmetry to the shape, but it is unclear if it is significant. The galaxy doesn't appear to be undergoing any major merger activity or experiencing intense star formation within the observed wavelengths.
