The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. There is little evidence of significant spiral arm structure or prominent dust lanes. The overall color is yellowish, suggesting a population of older stars with lower rates of ongoing star formation. The galaxy is largely spheroidal in shape, exhibiting a high degree of roundness. There are no obvious signs of a major ongoing merger or tidal disruption. The morphology suggests that it is a relatively isolated system that has likely undergone significant relaxation. There may be a very slight asymmetry present, hinting at a possible minor interaction in the past or a small infalling satellite. Overall, the galaxy seems to be a fairly typical elliptical at the observed redshift.
