The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. There is no discernible spiral structure. The light distribution suggests a concentrated central bulge that diffuses outwards into a less dense halo, as would be expected for an elliptical galaxy. The galaxy's color is skewed towards the redder part of the spectrum. This could be due to either the effects of redshift from its distance, and or an older stellar population, or internal dust absorption. There are some minor disturbances surrounding the central area. These could be caused by a minor interaction with another galaxy in the area. Further analysis using higher resolution imaging and spectral data is recommended to confirm these observations and determine the galaxy's precise characteristics.
