This galaxy appears to be an elliptical galaxy at a redshift of approximately 0.195, suggesting a significant distance from our own. The object exhibits a smooth, elongated morphology, displaying a cigar-like shape with a concentration of light in the central region, which likely hosts an older stellar population. The galaxy appears largely undisturbed, with no readily apparent signs of ongoing major merger activity or significant tidal disturbances. The red color suggests a relatively low rate of star formation compared to bluer galaxies. There may be some evidence of a disk-like structure, however this is not immediately clear.
