The galaxy presents as a concentrated, elliptical-like structure. Its color profile leans towards the redder end of the spectrum, suggesting an older stellar population. The smoothness of the light distribution indicates a lack of significant spiral arms or patchy star-forming regions. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. The moderate redshift suggests that it is a relatively distant object. The size appears to be small, possibly indicating that it is either a dwarf galaxy or a larger galaxy that is farther away. Its overall morphology suggests it is a passively evolving galaxy.
